The galaxy presents a primarily smooth morphology with a hint of a disk-like structure. It appears elongated, with a moderate degree of apparent roundness. No major mergers or significant disturbances are visually evident. Color gradients suggest some variation in stellar populations throughout the galaxy, with a relatively compact and centralized concentration of luminous matter. The overall light profile suggests a somewhat centrally concentrated object. There is a relatively faint but clear disk structure. The redshift implies that it is a relatively distant galaxy.
