The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears to be a yellowish-white hue, suggesting an older stellar population. The galaxy's overall form indicates a system that is not actively undergoing a major merger event; however, a slight irregularity in its outer structure could be interpreted as a minor disturbance. The overall rounded appearance suggests that it could be categorized somewhere between a more spherical and a more elliptical galaxy. There is some indication of light falloff from the inner center to its outer edges. 
