The galaxy presents as a relatively symmetrical elliptical morphology. It exhibits a centrally concentrated bulge that dominates the light profile. The bulge region appears smooth and featureless. Extending outwards from the core, a more diffuse halo is observed.

Color gradients are subtle, but present. The central bulge exhibits a yellowish-white hue, possibly indicative of an older stellar population. The outer regions of the galaxy appear slightly bluer, which could imply the presence of younger stars or a more active star forming region in those outer areas. The galaxy appears undisturbed, showing no obvious signs of tidal interactions or recent merger events.
