The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that is bright. The light profile appears to fade gradually from the center outwards, suggesting a lack of prominent spiral arms or distinct features. There may be some very slight flattening, but overall it looks round. It may be undergoing some minor mergers. The galaxy presents a redder hue, indicating an older stellar population with a potentially lower rate of current star formation.
