This galaxy exhibits an elliptical morphology, characterized by a relatively smooth and centrally concentrated light distribution. The color gradient suggests a dominant population of older stars, with the core region appearing more yellow-red. A lack of distinct spiral arms or prominent dust lanes is observed. There may be some tidal disturbances or a merging event, but is only slight. The overall shape appears somewhat elongated. The galaxy presents a redshift consistent with a significant cosmological distance, indicating an extragalactic source. Based on color and morphology, this galaxy is likely a relatively massive, passively evolving system with little ongoing star formation.
