The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light profile appears to gradually fade from the core outwards, exhibiting a relatively high degree of symmetry. The overall color is slightly bluer towards the outer regions than the center, which is more reddish-white, suggesting potential variations in stellar populations or dust content across the galaxy. There is no clear evidence of spiral arms, bars, or significant dust lanes visible in this observation. Faint, subtle irregularities in the outer regions may hint at minor interactions or disturbances. Based on its morphology, it is likely an early-type galaxy in the process of slow star formation.
