The galaxy presents as a generally smooth, elliptical morphology. It appears to be relatively featureless with no obvious spiral arm structures visible. The central bulge exhibits a bright, concentrated luminosity, suggesting a high density of stars and potentially a supermassive black hole actively accreting material. Moving outwards from the core, the luminosity gradually decreases, indicating a lower stellar density in the outer regions. The galaxy's shape is moderately elongated, exhibiting some deviation from perfect circularity. There are no apparent signs of recent major mergers or significant tidal disturbances, although subtle asymmetries or faint plumes could be present upon closer inspection. The overall color profile appears yellowish-red, indicating a population of older, cooler stars and relatively low levels of ongoing star formation. This color also suggests a higher abundance of heavier elements compared to younger, bluer galaxies. Based on its size and luminosity profile, this is likely a massive galaxy residing at a considerable cosmological distance.
