The galaxy presents as a luminous, concentrated object with a generally smooth appearance. It displays a moderate ellipticity. The core region is bright and yellowish-white, suggesting a population of older stars. The outer regions exhibit a slightly bluer hue compared to the core, hinting at the presence of a younger stellar population and possibly some ongoing star formation, although this is not strongly indicated. There is some indication of a disturbance in the light distribution in the galaxy’s morphology. The overall structure is consistent with a relatively massive galaxy at a non-negligible redshift.
