The galaxy appears to be an elliptical galaxy, with a smooth, concentrated light profile. It possesses a bright central bulge that dominates the overall luminosity. The galaxy exhibits a nearly perfect round morphology, with only a very slight deviation from circularity. The color gradient suggests a primarily older stellar population within the galaxy. There is no evidence of spiral arms or prominent dust lanes, or any major ongoing merging activity. The galaxy is likely a relaxed system. 
