The galaxy presents a generally smooth morphology, exhibiting a centrally concentrated light distribution. The overall shape appears elliptical, transitioning from a more rounded core to a slightly elongated outer region. A distinct color gradient is observed; the central region displays a yellowish-orange hue, indicative of an older stellar population. Moving outwards, a subtle shift towards a greenish tint suggests the presence of younger stars and possibly some ongoing, though limited, star formation in a ring structure. The outer regions fade into the background, indicating a gradual decrease in stellar density. There is no apparent evidence of major disturbances, tidal tails, or merging activity, suggesting it is a relatively quiescent system. The galaxy presents as a system with a large mass and low star formation.
