The galaxy presents as a largely featureless, elliptical-like structure. It exhibits a smooth, concentrated light profile. The core region displays a bright, yellowish-white hue, indicative of an older stellar population and minimal on-going star formation. There is a slight color gradient towards the outer edges, transitioning to a redder shade, which supports the dominance of older, redder stars in the galaxy's halo. There is no apparent evidence of spiral arms, a central bar, or significant dust lanes. The overall morphology appears undisturbed, with no obvious signs of recent mergers or tidal interactions.
