The galaxy presents as a relatively smooth, centrally concentrated elliptical, with a slight elongation in its morphology. It exhibits a mostly featureless disk with no significant dust lanes or spiral arm structure. The colour profile transitions gradually from a central yellow-white hue to more reddish tones in the outer regions. This suggests an older stellar population dominating the galaxy's composition, with potentially minimal ongoing star formation. The overall appearance indicates a mature galaxy that is not actively undergoing any major merging events, displaying a regular, settled structure.
