1 1226 C1 II Dust lane 2 1316 C1 0 Dust filaments. Nonthermal nucleus; saturated in g band 3 1978 II 4 881 C1 II Dust filaments. The surface brightness profile dips toward the center 5 798 C1: Y: II Possible dust patches. Visibly boxy within r<1". 6 763 C2 0 Dust lanes; nonthermal nucleus 7 731 Ib 8 1535 C3 0 Dust disk; visibly boxy in the inner region, disky at large radii 9 1903 Y Id Center saturated in g band; small inner stellar disk 10 1632 C1 II Dust filaments/patches 11 1231 Y: II Small nuclear bar? 12 2095 Y Ib ITD? 13 1154 C3 Id Dust Disk 14 1062 Id Evidence for distinct morphological components 15 2092 Ib Y 16 369 Ib Y: 17 759 C4 II Y Small nuclear dust disk; stellar rings, arcs 18 1692 Y Y Ic Edge-on stellar ring. 19 1030 C3 Y 0 Dust disk. Boxy isophotes in the inner region, disky at large radii 20 2000 Y Id Center saturated in g band; visibly boxy bulge superimposed to a disk component. Possible remnant of stripped satellite present in the field. 21 685 C4 Y Y 0 Dust disk; disk population of GCs 22 1664 Y Ic Disky isophotes 23 654 Ib Y Stellar ring; possible remnant of stripped satellite present in the field 24 944 Y Ic 25 1938 Y Ib ITD; possible spiral structure? 26 1279 Y Id 27 1720 Ia 28 355 C1 Id Y Dust filaments 29 1619 C1 Ia Dust filaments 30 1883 Ia Y 31 1242 Y Ia Large GC population 32 784 Ia Visible isophotal twists 33 1537 Id Y ITD? Small GC system 34 778 Id Y 35 1321 Id Visible isophotal twists 36 828 Ia Visibly boxy 37 1250 C3 Ia Dust disk 38 1630 Y Ia 39 1146 Y Ia 40 1025 Ic 41 1303 Ib Spiral arms 42 1913 Y Y Ia Distinct morphological components 43 1327 C4 Y II Dust disk. Tidally truncated by interaction with M87 44 1125 Y Y Ia ITD? 45 1475 Y Ib 46 1178 Ib 47 1283 Ia Y: 48 1261 Ia 49 698 Y Y Ia 50 1422 C1: Ia Possible large-scale dust filaments 51 2048 Y Ia 52 1871 Ia 53 9 Ie Low surface brightness 54 575 Y Y Id ITD or stellar ring 55 1910 Ia 56 1049 II 57 856 Ia Dwarf spiral 58 140 Ia 59 1355 Ia 60 1087 Ia 61 1297 Id Tidally truncated by interaction with M87 62 1861 Ia 63 543 Ia 64 1431 Ia 65 1528 Ia 66 1695 Ia Spiral pattern? 67 1833 II 68 437 Ia 69 2019 Ia 70 33 Ia 71 200 Ia 72 571 C2 0 Dust lane 73 21 Ie dIrr/dE transition 74 1488 Y Ia 75 1779 C1 Ie dIrr/dE transition, Dust filaments; small GC system 76 1895 Ia 77 1499 II dIrr/dE transition 78 1545 Ia Substantial population of bright clusters 79 1192 Ia Tidally truncated by interaction with M49 80 1857 Ie Low surface brightness 81 1075 Ia 82 1948 Ie 83 1627 Ia Small GC system 84 1440 Ia Large GC system 85 230 Ia 86 2050 Ia 87 1993 Ib 88 751 Y Ia 89 1828 Ia 90 538 Ia 91 1407 Ia Large GC system 92 1886 Ia 93 1199 Y Ia Spiral pattern? Tidally truncated by interaction with M49 94 1743 Ib 95 1539 Ia Large GC system 96 1185 Ia 97 1826 Ia Small GC system 98 1512 II dIrr/dE transition 99 1489 Ia 100 1661 Ia