The galaxy presents as a centrally concentrated spheroid with a high degree of smoothness. The light profile appears to be relatively uniform, lacking significant substructure such as spiral arms or prominent dust lanes. The core region exhibits a yellowish hue, possibly indicative of an older stellar population. The outer regions display a bluer coloration, potentially suggesting the presence of some younger stars, though their contribution appears minor given the overall color. There is no evidence of strong tidal features, major disturbances, or ongoing mergers. The overall morphology is consistent with an elliptical galaxy or a lenticular galaxy viewed face-on.
