The galaxy appears as a single, relatively smooth and concentrated object. There is a lack of obvious spiral arm structure or significant dust lanes. The morphology suggests an elliptical galaxy or perhaps a lenticular galaxy seen at a sufficient distance that finer details are obscured. The overall shape is approximately elliptical. The colouration is somewhat uniform across the galaxy, with a slight tendency towards redder hues, suggesting an older stellar population and lower levels of ongoing star formation. There are no signs of a major ongoing merger. Small perturbations cannot be ruled out. 
