The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that emits a yellowish-orange light, suggesting an older stellar population. There is little discernible evidence of spiral arms or distinct features. The outer regions of the galaxy fade gradually into the background, lacking sharp boundaries. A slight elongation is observable, hinting at a deviation from perfect circularity. The overall color profile indicates a potentially quiescent system with diminished star formation activity.
