The galaxy presents as an elliptical morphology with a smooth, concentrated light distribution. The core region exhibits a yellowish hue, suggestive of an older stellar population. A subtle gradient towards bluer colors is observed in the outer regions, potentially indicating the presence of younger stars or ongoing star formation at a low rate. The galaxy appears relatively undisturbed, showing no distinct signs of tidal interactions or major merging events. The overall appearance is consistent with a massive galaxy exhibiting minimal recent star formation.
