The galaxy presents as a centrally concentrated, relatively smooth object. It is largely elliptical in shape, appearing close to circular, with minor deviations from perfect roundness. There is a bright, prominent core that graduates into a diffuse halo. Faint, disturbed arm-like structures appear to extend from the central region of the galaxy. There is little evidence of spiral arm structure or active star formation. There is minor evidence of a potential merging event. The light profile suggests an older stellar population. Overall, the galaxy seems to be a quiescent system undergoing minor disturbances.
