The galaxy appears as a fairly smooth, centrally concentrated object with a largely elliptical morphology. There is a notable lack of spiral arm structure. The light distribution suggests a centrally dominant bulge component, with a gradual decrease in surface brightness towards the outer regions. The galaxy exhibits a yellowish-white hue, indicating a stellar population dominated by older, redder stars, possibly with ongoing, but subdued star formation. No obvious signs of tidal disturbances, major mergers, or prominent dust lanes are visible. The galaxy's roundness suggests a relatively low inclination angle with respect to our line of sight.
