The galaxy presents as a relatively smooth, centrally concentrated object. It is generally elliptical in appearance, with a high degree of radial symmetry. The central region exhibits a bright core that fades out into the surrounding galactic structure. There is little apparent evidence of spiral arms or a distinct disk component. The overall color is slightly bluer in the outer regions than in the inner regions. The galaxy appears to be isolated, with no obvious signs of tidal interactions or major mergers. Minor asymmetries are observed in the diffuse outer halo.