The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange, suggesting an older stellar population. The overall shape is fairly round. There is minimal evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively isolated, showing no prominent signs of tidal interactions or ongoing mergers, though some minor asymmetry can be observed to the left. The outer regions fade gradually into the background, indicating a diffuse halo. Star formation is likely low.
