The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a central, bright core, with a surrounding, diffuse halo. The overall shape is somewhat elongated, verging on cigar-shaped, although a rounder morphology cannot be ruled out due to the resolution. There is very little evidence of spiral arms or other distinct features usually associated with disk galaxies. There are no obvious signs of ongoing major mergers, although subtle disturbances in the outer regions cannot be entirely excluded. The color gradient shifts from a slightly bluer hue in the outer regions towards a yellower central region.
