The galaxy presents as a somewhat elliptical and compact structure. Its central region appears bright and relatively featureless, possibly indicating a significant bulge component or a dense concentration of older stars. The overall color appears yellowish-white, suggesting a relatively mature stellar population. There is some hint of bluer regions in the outer parts of the galaxy, which may be due to recent star formation activity, although these are not very prominent. The light distribution is smooth, suggesting the galaxy is likely an early-type spiral or elliptical galaxy. There seems to be little evidence of strong tidal interactions or major disturbances from mergers, although there could be minor features not resolvable at this resolution. Overall, the galaxy has a relatively simple and evolved morphology.
