The galaxy presents a generally elliptical morphology, with a high degree of central concentration. The core appears bright and almost unresolved, suggesting an older stellar population or possible active galactic nucleus. The outer regions of the galaxy exhibit a gradual decrease in surface brightness, indicating a smooth transition in stellar density away from the center. The color profile appears relatively uniform, with a subtle reddening in the central regions compared to the slightly bluer, fainter outskirts, which could be related to differences in the ages and metallicities of the stars in these areas. There is a subtle hint of a disk, but it is not as prominent as a spiral galaxy would have. The smooth profile and elliptical shape suggests a relatively evolved system with little ongoing star formation. There seems to be no evidence of recent major merger activity.
