The galaxy appears as a single, relatively smooth, elliptical-like object, exhibiting a concentrated central bulge that gradually fades into its outer regions. There is a slight elongation, but the overall form is largely rounded. The color profile suggests a predominantly older stellar population. Star formation is likely minimal or quiescent. It is possible there may be an additional very minor structure near the galaxy, perhaps from a minor disturbance or merger event. The galaxy appears to have no spiral arms. The overall structure appears largely undisturbed.
