This galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears bright yellow/white, suggesting an older stellar population. The outer regions of the galaxy fade into a more diffuse halo. There is little evidence of spiral arms or active star formation. Overall, the galaxy appears well-formed and undisturbed, showing no obvious signs of recent merger activity, and is fairly round. The color gradient suggests a relatively homogenous stellar population throughout the galaxy. The overall luminosity indicates a moderate absolute magnitude. The size seems relatively compact.
