The galaxy presents as a single, centrally concentrated object, likely an elliptical galaxy given the smooth light profile and apparent lack of spiral arms or a distinct disk component. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population or significant dust obscuration of bluer, younger stars. The galaxy's morphology appears relatively undisturbed, showing no obvious signs of ongoing or recent mergers or tidal interactions. There may be some slight elongation to the galaxy's shape, but it is largely rounded.
