The galaxy presents as a singular, centrally concentrated object. Its overall morphology appears smooth and relatively featureless. It has a roughly elliptical shape, appearing more elongated than perfectly circular. There is a subtle color gradient observed, with a slightly bluer hue towards the central region, possibly indicative of recent or ongoing star formation activity. No clear spiral arms or a distinct disk structure are discernible. There may be some minor disturbances or faint tidal features suggesting a past interaction or minor merger event. The galaxy seems to exist as a relatively isolated system.
