The galaxy appears as a single, centrally concentrated object with a smooth, featureless morphology. It exhibits a generally round shape, with a very slight elongation. The light profile suggests a relatively homogenous distribution with no apparent spiral arm structure or significant dust lane obscuration. The color gradient indicates a redder central region that shifts to a bluer hue in the outer regions. The overall color suggests a population of older stars with ongoing, but relatively subdued, star formation activity. There is no evidence of any major interaction with another galaxy or significant tidal disturbances; however, minor disturbances cannot be completely ruled out.
