The galaxy presents as a single, relatively smooth object with some asymmetry. A distinct color gradient is observed, transitioning from a bluer hue on the left side to a yellower, more concentrated center on the right. The morphology suggests an elliptical classification, though the blue tint on one side indicates the presence of a region of star formation, giving it a hybrid nature. This asymmetry could result from a minor gravitational disturbance, possibly related to a companion galaxy not visible in this image, or internal processes. The galaxy is moderately luminous, and the size appears consistent with a typical massive galaxy at its redshift. There are no easily observable features such as spiral arms or prominent dust lanes.
