The galaxy presents as a relatively smooth, elliptical form. Its color profile is generally yellowish, suggesting a population of older stars. There is a slight elongation to the galaxy's shape; it is not perfectly circular. There are no obvious signs of spiral arms or significant dust lanes. No active galactic nucleus is apparent in the available imagery. There are no indications of ongoing major mergers or tidal disturbances. The galaxy appears to be an isolated system with no nearby companions visibly interacting with it.
