The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, which transitions smoothly to a less dense, extended halo. The core region displays a yellowish-white hue, indicative of an older stellar population. The halo exhibits a bluer tinge. There is no apparent spiral structure or dust lanes visible. The overall shape is somewhat elongated. No signs of tidal tails, merging activity, or significant morphological disturbances are apparent. Based on its color and morphology, this galaxy appears to be a relatively evolved system with a dominant older stellar population and a low star formation rate.