The galaxy presents as a centrally concentrated, smooth structure. It exhibits a largely elliptical morphology, appearing nearly circular in projection. There is a clear color gradient, with a yellowish core transitioning to a bluer outer halo. No distinct spiral arms or prominent dust lanes are apparent. The galaxy appears relatively isolated, showing no signs of major tidal disturbances or ongoing mergers based on its morphology. The surface brightness profile suggests a centrally dominant bulge. Evidence suggests that the star formation is relatively low and that this is a massive galaxy.
