The galaxy presents as an elongated, likely elliptical, structure. Its core exhibits a bright, concentrated region suggesting a high density of stars and potentially an active galactic nucleus. The overall color profile indicates a population of older stars, with a redder hue dominating the central region. However, there are hints of bluer patches along the periphery, suggestive of ongoing or recent star formation activity. The morphology does not immediately reveal any significant tidal disturbances or interactions, though a slight asymmetry in its shape is observed. Given its considerable luminosity and inferred stellar mass, this galaxy is likely a massive system residing at a cosmological distance, and thus its physical size is considerable. The light observed is from when the universe was significantly younger.
