The galaxy presents a relatively smooth, elliptical morphology. It displays a concentrated central bulge, which dominates the overall light profile. The light from the galaxy is yellowish-orange, suggesting a stellar population that is dominated by older stars. There is little evidence of spiral arms or significant dust lanes. The galaxy appears to be a fairly relaxed system, without any major signs of ongoing mergers or strong tidal disturbances. It is not perfectly round, but rather slightly elongated.
