The galaxy presents as a relatively smooth, centrally concentrated object with a moderate ellipticity. Its overall color appears yellowish-white, indicating a stellar population that is likely dominated by older, evolved stars, and potentially lower levels of ongoing star formation. There is a brighter core region that gradually fades into the outer regions of the galaxy. There's no evidence of spiral arms or significant dust lanes. The morphology suggests it could be an elliptical galaxy or a lenticular galaxy seen at a slight inclination. There may be some minor disturbances within the galaxy, but it mostly exhibits a relaxed structure, meaning that any past interactions were likely minor or are already well-integrated into the galaxy's current form.
