The galaxy appears as a single, concentrated, symmetrical object. There is little to no evidence of spiral arms or a distinct disk structure; the light is smoothly distributed. The galaxy is largely featureless, exhibiting no strong dust lanes or prominent star-forming regions. It presents a largely elliptical morphology, with a round shape. There are no obvious signs of ongoing major mergers or significant tidal disturbances. The galaxy's color suggests a population of older stars, with lower levels of active star formation.
