The galaxy appears to be a relatively smooth, elliptical or lenticular type, with a dominant central bulge. There is little to no visible dust or spiral arm structure. The galaxy exhibits a slightly elongated shape, appearing more "in-between" round and cigar-shaped. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. No signs of major merging activity are discernible, although minor disturbances cannot be ruled out. The overall color suggests a population of older stars, with a somewhat redder hue. The galaxy seems to be isolated, residing in a field with a relatively low density of other visible objects.
