The galaxy presents as a centrally concentrated object with a smooth, generally elliptical morphology. The core region appears bright and slightly yellow-white, with the light intensity diminishing gradually towards the outer regions. There is minimal evidence of distinct spiral arms or significant dust lanes, suggesting a relatively uniform distribution of stars. The shape tends to the rounder side of being elliptical. There are hints of faint, diffuse extensions beyond the main body of the galaxy, potentially indicative of a halo component. No obvious signs of a major ongoing merger are detected, though minor asymmetries or distortions in the outer regions cannot be entirely ruled out. The galaxy appears to be fairly evolved.
