The galaxy presents as a single, relatively smooth structure with a concentrated central bulge. Its overall color is yellow-orange, potentially indicating an older stellar population. The light profile appears generally elliptical, with a high degree of roundness. There is very faint suggestion of a disk, but the overall morphology is dominated by the smooth bulge. There is no visible evidence of spiral arms or significant dust lanes. There are no obvious signs of ongoing mergers or tidal disturbances, the galaxy seems to be fairly settled and undisturbed.
