The galaxy presents as a relatively smooth, centrally concentrated structure. It exhibits a slight elliptical morphology, appearing more 'in-between' than round or cigar-shaped. Some bluer hues can be seen in a diffuse disk with hints of structure or a few fainter arms. There is no strong indication of a recent major merger event, although subtle irregularities suggest minor disturbances may be present. The central region is more luminous than the surrounding area, and the color suggests older stars, with an estimated stellar mass that is typical. Its estimated star formation rate is low.
