The galaxy presents as a single, relatively smooth object. It is somewhat elliptical, displaying an intermediate roundness, between circular and elongated. The core appears to be quite bright and concentrated, with a yellow-orange hue. Fainter, bluish extensions emanate from the central region, potentially indicative of a disk-like structure with some level of star formation. There are no immediately apparent signs of major tidal disruption or ongoing merger events. The overall color gradient suggests a population of older stars dominating the central bulge, while younger stars might be present in the fainter, bluer outer regions. The galaxy seems to be in a relatively quiescent state.
