The galaxy presents as a centrally concentrated elliptical or lenticular morphology. It has a smooth, diffuse appearance with no discernible spiral arm structure or prominent dust lanes visible. The central region exhibits a yellow-orange hue, suggesting a population of older stars. The outer regions appear slightly bluer, but this is not pronounced, indicating minimal recent star formation. The overall shape is close to circular, with only a slight elongation. There is no evidence of tidal features, mergers, or significant disturbances, and the galaxy appears relatively isolated. The galaxy is compact, with the light concentrated towards the core.
