The galaxy presents as a relatively smooth, centrally concentrated object. Its overall color appears yellow, suggesting an older stellar population. There may be a slight extension that isn't perfectly circular, more in between in shape. No prominent spiral arm structures or significant dust lanes are visible. The smooth appearance indicates that the galaxy is unlikely to be undergoing a major merger. Based on the object's morphology, it may be an elliptical galaxy or a lenticular galaxy with a relatively low star formation rate, confirmed by its high-mass and low rate of star formation. Evidence of only minor disturbances is seen. 
