The galaxy presents as an edge-on spiral with a prominent central bulge. The bulge exhibits a smooth, somewhat boxy morphology, suggesting a significant population of older stars. The disk appears thin and elongated, characteristic of edge-on orientations. There is faint evidence of spiral structure within the disk, but the edge-on view obscures detailed arm features. Dust lanes are not readily apparent, though some subtle color variations suggest obscuration in the disk. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major merging activity, though a minor interaction cannot be ruled out. The galaxy exhibits a substantial mass and moderate star formation activity within the disk. The colour gradient suggests a range of stellar populations, with redder colours concentrated towards the bulge.
