The galaxy presents a generally smooth, elliptical morphology. The central region displays a concentrated, bright yellow hue, suggesting a population of older, evolved stars. Moving outward from the center, the light gradually diminishes. A faint disk can be tentatively identified, oriented roughly horizontally. There appears to be some minor asymmetry in the outer regions, potentially indicating a past interaction or disturbance. The overall color gradient from the central bulge to the outer regions suggests ongoing or recent star formation, albeit at a relatively low rate, as the galaxy appears to be populated by an older stellar population. 
