The galaxy appears to be an early-type spiral, possibly an S0 or Sa galaxy, viewed nearly edge-on. A bright, extended bulge dominates the central region, with a relatively uniform luminosity distribution and color suggesting an older stellar population. Faint hints of a disk are visible extending beyond the bulge, with a slight flattening toward the edges. There might be some minor disturbances or asymmetries, potentially suggesting a past interaction or minor merger. Faint color variations are observed within the bulge, with slightly bluer regions possibly indicating younger stellar populations mixed with older ones. The disk appears to be relatively smooth with no obvious spiral arm structures. The overall color profile suggests the galaxy is relatively evolved.
