The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall shape appears to be elliptical, displaying a slight elongation. There's minimal indication of spiral arm structures. The light distribution is somewhat even, fading gradually outwards from the core. The color profile suggests a population of older stars, with a redder hue, although there is a trace of blue. There are no obvious signs of ongoing major mergers or significant tidal disturbances, though the presence of subtle irregularities cannot be entirely ruled out.
