The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a concentrated central bulge that is brighter than the surrounding halo. The color distribution is consistent with a population of older stars, with a slightly redder hue in the central regions transitioning to a bluer color at the edges. There is no obvious spiral structure or prominent dust lanes visible. The galaxy has a round appearance with no signs of major mergers. There appears to be slight disturbances in the surrounding regions of the halo.