The galaxy presents as a luminous, centrally concentrated object with a smooth overall morphology. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. The outer regions display a more diffuse reddish tint, possibly indicative of ongoing or recent star formation within dusty regions, though at a low rate. The galaxy appears largely spheroidal with a high degree of circular symmetry, with no apparent spiral arms or significant morphological disturbances. The overall appearance indicates a massive galaxy at a substantial cosmological distance. There is no evidence of any major merger events or tidal interactions with neighboring galaxies.
