The galaxy presents as a centrally concentrated object with a largely smooth and featureless appearance, indicating an elliptical morphology. The light is relatively uniformly distributed, exhibiting a high degree of central concentration, with no discernible spiral arms or bar structures. The overall shape is quite round, with the light appearing somewhat diffused toward the outer edges. There is subtle evidence of a slight disturbance in its morphology, but the general structure shows no ongoing major merging activity. The observed color suggests a galaxy composed of an older stellar population, consistent with low current star formation, and a resulting redder hue overall. The size appears to be of a moderate physical scale, given its estimated redshift.
