The galaxy appears to be an elliptical galaxy. It presents as a relatively smooth, centrally concentrated object with a diffuse halo. The central region exhibits a yellowish-white hue, suggesting an older stellar population. There is a slight elongation visible. There are no obvious spiral arms or significant dust lanes visible. The outer regions seem to fade gradually into the background, and there is no indication of any major ongoing merger events, although some minor tidal disturbances cannot be completely ruled out.
