The galaxy presents as a relatively smooth, centrally concentrated object. The dominant color appears to be a yellowish-white hue, potentially indicative of an older stellar population. There is a hint of a redder component on one side of the galaxy, but it appears minor. The overall morphology suggests an elliptical galaxy or a lenticular galaxy viewed face-on. There is no obvious indication of spiral arms or significant dust lanes. There is no obvious merging or recent major disturbances, but some minor disturbance may be affecting the galaxy. Based on the overall color and morphology, the galaxy does not appear to be actively forming many stars. The round appearance suggest that it may be nearing the end of any transformation processes and is relatively stable.
