The galaxy presents as a concentrated, elliptical-like structure. It exhibits a smooth, largely featureless appearance with a dominant central bulge. The color profile suggests a population of older stars, trending towards the redder end of the spectrum, with a yellow-orange hue across its body. There is no obvious dust lane or spiral arm structure visible in this image. The overall morphology appears relatively undisturbed, with no indications of a recent major merger or tidal disruptions. Based on the high redshift, the galaxy is observed at a significant distance, which causes the galaxy to appear small. The light is also shifted towards the redder end of the spectrum, implying that it is moving away from the observer.
