The galaxy presents as a centrally concentrated, smooth structure, likely an elliptical galaxy at moderate redshift. Its morphology appears largely undisturbed, exhibiting a centrally concentrated nucleus with a yellowish-orange hue, indicating an older stellar population. The light gradually fades outwards from the core, transitioning to a faint, diffuse halo with hints of a bluer component suggesting a small amount of ongoing star formation. The galaxy's overall form is generally elliptical, appearing somewhat in between round and elongated, without any pronounced spiral arms or obvious signs of a major merger event, although there might be a minor disturbance affecting the morphology.
