The galaxy appears to be a relatively smooth and round elliptical galaxy. The galaxy exhibits a concentrated central bulge that fades into a more diffuse halo. There is a slight elongation, but overall the object's shape is fairly circular. There is some evidence of a faint, disturbed feature, like a tidal tail, on one side of the object, suggesting the galaxy may have undergone a minor merger. No prominent spiral arms or distinct dust lanes are visible. The color gradient suggests an older stellar population, with light becoming redder moving from the center to the outer edges.
