The galaxy presents as a relatively smooth and centrally concentrated object. It exhibits an elliptical morphology, though it tends towards an intermediate roundedness, departing slightly from a perfectly circular appearance. There is a suggestion of a central bulge, indicated by a brightening in the core region. The overall color appears to be consistent with an older stellar population, with redder hues. No prominent spiral arms or significant dust lanes are visible. The galaxy does not appear to be undergoing any major merger activity, though there is a slight indication of minor disturbances in the outer regions.
