The galaxy presents as a relatively compact, elliptical system. It exhibits a smooth, centrally concentrated light profile, with minimal visible substructure. The galaxy's color suggests a predominantly older stellar population, lacking significant ongoing star formation. The round morphology further supports its classification as an elliptical galaxy. There is no indication of tidal features or interactions with other galaxies, implying it is currently isolated or has undergone recent relaxation processes. The galaxy's overall appearance indicates a mature system with a substantial stellar mass and low specific star formation rate.
