The galaxy appears to be a relatively smooth, centrally concentrated system, exhibiting a generally elliptical morphology. The core region is bright and somewhat diffuse, with a gradual decrease in luminosity extending outwards. Some slight disurbances can be observed at the outer edge. The galaxy has a relatively uniform color gradient, hinting at a more evolved stellar population. Based on these observations, the galaxy could be an elliptical, or possibly a lenticular galaxy seen face-on.
