The galaxy presents a smooth, elliptical morphology with a centrally concentrated luminosity profile. The core region exhibits a bright, yellowish-white hue, indicating a population of older stars. The isophotes appear relatively regular and undisturbed, suggesting a lack of recent major merger events. There is a slight elongation, indicating a deviation from perfect circularity, but no pronounced disk-like structure is discernible. The outer regions of the galaxy fade gradually into the background, exhibiting a redder color than the core. There is no visible evidence of strong star formation, spiral arms, or significant dust lanes. The overall appearance is consistent with that of an early-type galaxy, potentially an elliptical or lenticular galaxy at a considerable redshift.
