The galaxy presents as a somewhat diffuse, yet luminous object. It exhibits a moderately elliptical morphology, appearing more 'in between' than perfectly round, with no discernible spiral arm structure. The galaxy exhibits a smooth appearance, with no obvious dust lanes or distinct star-forming regions visible in the image. There are signs of tidal disturbance suggesting that this galaxy is interacting with one or more neighboring galaxies. Color gradients are present, with a slightly bluer core region transitioning to redder outer regions. This could indicate a difference in stellar populations, with younger stars dominating the central region. The redder color in the outskirts may be due to older stars or dust obscuration. The overall impression suggests an evolving galaxy possibly undergoing a merger event.
