The galaxy presents as a relatively compact, elliptical-like structure. The light distribution appears smooth and concentrated, indicative of an older stellar population. There is a lack of prominent spiral arms or dust lanes that are characteristic of disk galaxies. The color gradient transitions from a yellow-orange core to a slightly bluer halo, suggesting some recent star formation activity, but likely at a low rate. The round appearance and lack of significant tidal features suggest it has likely not undergone a recent major merger, though there is the possible presence of minor disturbances or interaction. There is evidence of possible merging with another object. The redshift is significant, indicating that we are observing this galaxy at a considerable distance. Overall, this galaxy is likely a relatively massive system with a substantial population of older stars.
