This galaxy appears to be an elliptical galaxy at a distance indicated by its redshift. It exhibits a smooth, centrally concentrated light profile with a high degree of symmetry. The shape is somewhat elongated. The central region displays a yellowish hue, likely indicative of an older stellar population. The outer regions transition to a bluer color, which could imply the presence of some younger stars, although star formation is expected to be low. There are no obvious spiral arms, dust lanes, or signs of recent major mergers. The galaxy seems relatively undisturbed and isolated.
