The galaxy presents as a relatively smooth, centrally concentrated object, elliptical in appearance. Its color profile exhibits a yellow-white hue, suggestive of an older stellar population, although the presence of bluer regions cannot be ruled out due to the resolution of the image. The light distribution decreases gradually from the center outwards, without any sharp breaks or distinct spiral arm features. There is some asymmetry visible in the outer isophotes, with a slight extension in one direction. The galaxy appears relatively isolated, lacking obvious signs of recent major merger activity, although some evidence of minor disturbances cannot be discounted. The galaxy is not perfectly round, but closer to a round profile than cigar shaped.
