The galaxy presents an elliptical morphology with a smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish-orange hue, suggesting a population of older stars. The light intensity gradually decreases from the center outwards, forming a diffuse halo with no distinct spiral arm structure or prominent dust lanes visible. The galaxy appears relatively undisturbed, without any obvious signs of recent major merger events. There may be some minor disturbance but the light is overwhelmingly smooth. The color gradients suggest a radial change in stellar population or metallicity, with the outer regions appearing slightly bluer than the core, hinting at the presence of some younger stars, albeit in small quantities. Overall, the galaxy's features are consistent with a massive, early-type galaxy at a significant redshift.
