The galaxy presents as a largely featureless elliptical or lenticular galaxy. It appears to be relatively smooth and uniformly colored, with a centrally concentrated bulge. The color gradient suggests a population of older stars. The absence of distinct spiral arms or significant dust lanes supports the classification as either elliptical or lenticular. There is a slight elongation observable, with the long axis significantly greater than the short axis, indicating it is cigar shaped. There are no visible signs of a major merger or tidal disturbances in this image, though a minor disturbance cannot be ruled out.
