The galaxy presents as an elliptical morphology, displaying a smooth, concentrated central bulge that appears to be nearly symmetrical. There is no visible dust lane or spiral arm structure in the imagery. The galaxy has a color gradient, shifting from a yellow-white hue at its core to a faint, reddish outer halo, which may indicate an aging stellar population throughout the galaxy. The overall shape suggests a system that is transitioning toward being mostly supported by random stellar motions rather than a clear disk-like rotation. 
