The galaxy presents a generally smooth morphology, appearing largely featureless. Its overall shape is elliptical, exhibiting a slight elongation. The light distribution indicates a bright central bulge, potentially an indication of a supermassive black hole. The color gradients suggest a population of older stars, particularly in the central regions, with a subtle shift towards bluer hues in the outer regions indicating the possible presence of some younger stellar populations. There is no indication of tidal tails or other signs of recent mergers or significant interactions. The galaxy's color profile hints that star formation is present, but that the bulk of the galaxy is comprised of older stars. 
