The galaxy presents as a relatively smooth, elliptical structure, displaying a concentrated central bulge that gradually diffuses outward. There is a slight elongation noticeable in its shape, hinting at a classification between a perfect sphere and a more cigar-shaped form. Some minor disturbances are visible, but appear to be somewhat smooth still. The galaxy exhibits a color gradient, with the core appearing more yellow-white, possibly indicating an older stellar population, transitioning to a bluer hue in the outer regions, suggesting some ongoing star formation, but not in large quantities. The overall light distribution is centrally concentrated, lacking prominent spiral arms or distinct features.
