The galaxy presents as a smooth, elliptical structure with a high degree of central concentration. Its color is predominantly yellowish-orange, indicating a population of older stars with lower rates of on-going star formation. The galaxy exhibits a moderate ellipticity, appearing somewhat flattened along one axis. There is no discernible spiral arm structure or dust lane features visible. The overall morphology suggests an evolved system, likely a massive elliptical galaxy residing at a considerable cosmological distance. There are no obvious signs of recent merger activity or significant tidal disturbances affecting its morphology. The galaxy appears relatively isolated and undisturbed.