The galaxy presents a largely smooth morphology, with a structure tending towards elliptical. The central region exhibits a concentrated luminosity, appearing bright and slightly yellowish. Moving outwards from the core, the intensity gradually decreases into a more diffuse halo. Hints of a flattened, disk-like structure may exist, but the smoothness dominates. There is a subtle bluer color towards the outer edges indicating possible star formation. The galaxy appears to be relatively isolated with no obvious signs of interaction or ongoing merger activity, though there are minor disturbances, but they are not overly distorted. The general shape is somewhere between round and elongated.
