The galaxy presents as a somewhat elongated, centrally concentrated light source. The core region exhibits a bright, yellowish-white glow, suggesting a population of older stars and potentially an active galactic nucleus. A diffuse, fainter halo surrounds the central region, showing a slight reddish hue further from the center, indicative of a declining star formation rate within these outer regions. The overall form appears relatively undisturbed, with no obvious signs of major mergers or significant tidal interactions. It is characterized by a smooth morphology. The apparent size suggests that it is a moderate-sized galaxy at its redshift.
