The galaxy presents a largely smooth and rounded morphology, characteristic of an elliptical galaxy. The light is centrally concentrated with a fairly uniform luminosity gradient outward from the core. The galaxy exhibits a yellowish hue, suggesting an older stellar population dominates the light emission. There is no discernible spiral structure or dust lane visible. The overall appearance indicates a relatively quiescent galaxy, with little evidence of ongoing major star formation or significant merger activity. There is a very slight reddishness on the outskirts of the galaxy.
