The galaxy appears as a centrally concentrated object with a smooth, somewhat elliptical morphology. The central region exhibits a yellowish-white hue, suggesting a population of older stars. The outer regions appear fainter and slightly bluer, which may indicate ongoing star formation, albeit at a low rate. There is no discernible spiral arm structure or bar feature. The overall structure suggests a galaxy somewhere between a pure elliptical and a lenticular type. There might be slight disturbances visible which could be interpreted as possible minor interactions.
