The galaxy presents as a relatively smooth object with a centrally concentrated luminosity profile. There is a distinct, bright core that gradually fades outwards into a more diffuse halo or bulge. The overall shape appears to be close to round, with minimal evidence of a distinct disk or spiral arm structures. There is no strong indication of recent or ongoing mergers or tidal disturbances. Color gradients are subtle, with a suggestion of a redder hue in the outer regions compared to the bluer, brighter central core. The galaxy appears to be a spheroid or an early-type spiral galaxy viewed face on at a considerable distance.
