The galaxy presents as a fairly smooth, elliptical-like object. It exhibits a concentrated central bulge with a gradual decrease in luminosity extending outwards. There is no distinct disk structure apparent; the light distribution appears relatively uniform and symmetrical. The color profile suggests a population of older stars, indicated by the reddish-yellow hue in the central regions. The outer edges appear bluer, suggesting the presence of some younger stellar populations or ongoing, albeit subdued, star formation activity. There is a slight asymmetry in the light distribution, possibly indicative of a past minor merger or tidal interaction. No prominent dust lanes or spiral arms are visible. The overall morphology suggests a galaxy in a relatively quiescent stage of evolution.
