The galaxy appears as a single, centrally concentrated object. The light distribution suggests a smooth morphology, with no obvious spiral arms or other distinct features. The radial color gradient indicates a slightly yellowish central region, fading to a bluer hue at the outer edges. It is generally elliptical in shape with no signs of active merging or major disturbances. The lack of defined structural features indicates a more evolved stellar population throughout the galaxy. The roundness of the galaxy is notable and is very clearly not cigar shaped. There are no visible dust lanes or regions of intense star formation.
