The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a subtle color gradient from the center outwards, transitioning from a yellowish-orange core to a slightly bluer halo. There is little indication of spiral arms or prominent dust lanes; however, its disk or halo extends beyond the central core with what appears to be an even distribution of older stars. There are no signs of major ongoing mergers or significant tidal disturbances, although subtle asymmetry may suggest possible minor interactions. Its overall visual impression is one of a mature, evolved system.
