The galaxy presents as a flattened elliptical form, displaying a dominant, smooth morphology. The central region exhibits a high degree of concentration, appearing bright and yellowish-orange. The outer regions transition into a less intensely colored halo with subtle greenish hues. There are no obvious spiral arm structures or significant dust lanes visible. The overall appearance suggests a relatively evolved system with ongoing, but potentially low, star formation activity. Subtle distortions in the outer halo may indicate past minor interactions or disturbances.
