The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high stellar density and possibly a supermassive black hole actively accreting material at its center. The galaxy's light profile appears to fade gradually from the center outwards, showing a somewhat diffuse halo. There appears to be little to no evidence of prominent spiral arms or significant dust lanes. Its color is primarily yellowish with hints of red, indicating a population of older, cooler stars. There are no obvious signs of active star formation, merging events, or significant tidal disturbances. The galaxy appears to be relatively isolated and undisturbed. Overall, the galaxy is a luminous, early-type galaxy at a significant cosmological distance.
