The galaxy presents as a relatively smooth, centrally concentrated object. Its overall morphology appears elliptical, exhibiting a high degree of sphericity. There is a suggestion of a slight elongation along a particular axis, but the galaxy is mostly rounded. A discernible color gradient is observed, with the central region exhibiting a yellowish-red hue, possibly indicating an older stellar population. The outer regions display a bluer color, which could be due to recent star formation activity. However, overall the object seems to be relatively quiescent. No apparent signs of strong tidal interactions or major mergers are observed.
