The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, with a gradual decrease in luminosity towards its outer regions. There is little to no indication of spiral arm structure or prominent dust lanes. The galaxy appears generally round in shape, with only subtle deviations from perfect circularity. Color gradients suggest an older stellar population, potentially with less ongoing star formation activity. No obvious signs of mergers or major disturbances are present. Overall, the galaxy appears as a well-formed, undisturbed system.
