The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse appearance. Its overall shape is roughly elliptical, exhibiting a high degree of roundness. There's a subtle color gradient; a slightly yellowish core fades into a bluish-white halo, suggesting variations in stellar populations. No distinct spiral arms or other disk-like structures are apparent, but there is the slightest hint of a disk shape to the galaxy. There's no indication of ongoing major mergers or tidal disturbances, though subtle asymmetries or faint extensions cannot be ruled out without higher resolution imaging. The overall morphology suggests an early-type galaxy, possibly an elliptical or lenticular galaxy that has undergone significant internal evolution, leading to a reduction in star formation.
