The galaxy presents an elliptical morphology, though some features suggest the presence of a disk. The central region appears bright and concentrated, suggestive of a prominent galactic bulge or core, with older stellar populations dominating the light emitted from this region. The outer regions exhibit a more diffuse appearance, with some indication of a faint, flattened disk component, possibly containing younger stars and ongoing star formation. The color distribution indicates a redder central region and a subtly bluer outer disk, consistent with differences in stellar populations. There are no obvious signs of strong tidal disturbances or recent major mergers, though there may be subtle signs of minor interactions. The galaxy seems relatively isolated.
