The galaxy presents as a luminous, elliptical-like object with a smooth and concentrated central bulge. The core is noticeably brighter, appearing nearly white, suggesting a high density of older stellar populations or potential active galactic nucleus activity. A yellowish hue surrounds the central region, indicative of evolved stars. The outer regions fade gradually into the background sky, forming a diffuse halo. No distinct spiral arm structures are discernible. Slight asymmetry in the outer envelope may suggest past interactions or minor disturbances. The overall morphology points to a mature galaxy with suppressed star formation.
