The galaxy exhibits a distinct edge-on morphology. It appears as a flattened, elongated structure, indicative of a disk galaxy viewed from the side. A prominent central bulge is visible, displaying a smooth and rounded profile. The bulge dominates the central region, with its luminosity gradually decreasing towards the outer disk. The disk appears relatively smooth, with some faint features that may be indicative of spiral arm structure or dust lanes. The overall color of the galaxy is consistent with an older stellar population, with a tendency towards redder hues. There is no evidence of significant merging or major tidal disturbances.
