The galaxy appears to be a relatively face-on spiral or lenticular galaxy. It exhibits a centrally concentrated bulge that is slightly reddish in color, suggesting an older stellar population. Fainter spiral arm structures appear to emanate from the central region and contain pockets of bluer light, possibly indicating areas of active star formation. The outer regions of the galaxy fade into the background, indicating a gradual decrease in stellar density. Overall the galaxy appears mostly smooth, with only some minor disturbances potentially visible.
