The galaxy appears to be a relatively smooth, elliptical-type galaxy at a considerable distance. It has a centrally concentrated bulge, exhibiting a yellowish-orange hue. The outer regions of the galaxy appear fainter and display hints of a bluer color, which may indicate the presence of a younger stellar population in the outer disk. There are no clear signs of spiral arm structures, and the overall shape is somewhat rounded, but it seems to extend more in one direction than the other. No major disturbances or mergers are apparent, though there might be a hint of minor disturbance visible.
