The galaxy presents as a centrally concentrated object with a smooth light distribution. Its overall shape appears to be elliptical, exhibiting a moderate degree of elongation. There is a slight color gradient visible, with the central region appearing more yellow, suggesting an older stellar population, while the outer regions appear slightly bluer. The galaxy displays no prominent spiral arm structures or significant dust lanes. There appears to be some minor asymmetrical light distribution in the outskirts, potentially indicating a minor disturbance. There is no indication of a major merger event or tidal tails.
