The galaxy presents as a concentrated, centrally brightened system. It exhibits a generally elliptical morphology with a high degree of circularity. The light is fairly smooth and diffuse, lacking any prominent spiral arm structures or distinct dust lanes that would indicate significant ongoing star formation or a disk component. There is a hint of a slightly elongated halo or outer region, but its features are faint and blend into the background sky. Overall, it resembles an elliptical galaxy at moderate redshift.
