The galaxy presents as a singular, dominant object, appearing generally smooth in texture and elliptical in shape. Its central region is marked by high luminosity, exhibiting a bright, concentrated core, indicative of a high stellar density or an active galactic nucleus. The light profile decreases gradually from the core outwards. There is little evidence of spiral arm structures or significant dust lanes. The overall color suggests a population of older stars, leaning towards redder wavelengths. There's potential evidence of a minor tidal disturbance, but for the most part it seems to be undisturbed.
