This galaxy presents as a relatively smooth, elliptical or lenticular system. It exhibits a concentrated central bulge that dominates the overall light profile, surrounded by a fainter, more diffuse halo. The galaxy's shape appears generally round. There are no readily apparent spiral arms or prominent dust lanes. Color gradients suggest a population of older stars. The galaxy does not obviously appear to be undergoing a major merging event or experiencing significant tidal disturbances. 
