The galaxy presents as a relatively smooth, rounded structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. No distinct spiral arms or bar structures are readily apparent. The color profile suggests a population of older stars, with a bias towards redder wavelengths and a low rate of star formation. The galaxy appears undisturbed, with no visual evidence of tidal interactions or ongoing mergers. It is likely an elliptical galaxy, or possibly a lenticular galaxy viewed face-on.
