The galaxy presents as a centrally concentrated object with a generally smooth appearance, indicative of an elliptical morphology. It exhibits a relatively compact core region that transitions into a more diffuse halo. The color profile is largely dominated by yellow hues, with some evidence of a green tint near the edges, suggesting moderate levels of recent star formation. There is no strong evidence of spiral arms or a prominent disk structure. The overall shape appears nearly round, showing little elongation or distortion which suggests a relaxed system that is not undergoing significant merger activity. The limited detail implies a substantial distance, and this is further supported by the high redshift indicating it is a relatively distant object.
