The galaxy presents as a generally smooth, elliptical structure with a centrally concentrated bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or distinct features. The overall color index suggests a population of older stars, with a tendency towards redder hues particularly noticeable in the outer regions. A slightly bluer region is seen toward the left edge of the galaxy. There is no obvious evidence of an ongoing major merger event, although a minor disturbance cannot be entirely ruled out. The galaxy exhibits a moderate degree of ellipticity, appearing more "in-between" than perfectly round or cigar-shaped. 
