The galaxy presents as a primarily smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. The overall color appears to be a slightly yellow hue, suggesting a population of older stars. The galaxy appears to be fairly round in shape, with little deviation from a spherical form. There is no immediately apparent evidence of a recent or ongoing major merger event, nor is there any obvious indication of spiral arm structures or a prominent disk component. There is no apparent presence of prominent dust lanes or gas clouds.
