The galaxy presents a generally smooth, elliptical morphology. It is dominated by a centrally concentrated bulge that appears nearly spherical in projection. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a reddish hue, suggestive of an older stellar population. The overall light profile appears fairly regular, with no obvious signs of strong tidal interactions or recent major mergers. There is a very slight asymmetry with some apparent light extending on one side. This may be due to a minor disturbance, possibly a small merger that is undetectable through visual inspection. The light is fairly uniformly distributed.
