The galaxy appears as a relatively smooth, centrally concentrated object with a somewhat elliptical shape. There is a slight elongation, but it is largely rounded in appearance. A gradual decrease in luminosity extends outward from the core, but no distinct spiral arms or detailed structures are readily visible. The color suggests that it is possibly dominated by an older stellar population. There are no obvious signs of recent major merger activity, although there is the possibility of a minor disturbance in its overall structure. The overall morphology suggests this galaxy is an elliptical or lenticular type.
