The galaxy presents a largely smooth, elliptical morphology. It appears centrally concentrated with a relatively high degree of circularity. There is a minor asymmetry present, possibly indicating a subtle interaction or disturbance. The galaxy exhibits a fairly uniform color gradient, with the core appearing slightly bluer than the outer regions. It displays a moderate red shift suggesting its at a considerable distance and there are no distinct spiral arms or obvious dust lanes are discernible. Its low star formation rate is consistent with its classification as an elliptical galaxy. There is no evidence of an active galactic nucleus or starburst activity. The galaxy appears relatively isolated, with no nearby companions readily apparent.
