The galaxy presents a primarily smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggestive of a high stellar density or possible active galactic nucleus. The light distribution appears radially symmetric and gradually diminishes toward the outer regions of the galaxy. A faint halo of diffuse light surrounds the main body, potentially indicating the presence of an extended stellar population. No distinct spiral arms or prominent dust lanes are observed, consistent with an early-type classification. Faint, asymmetric light structures appear in the outskirts, possibly a sign of a minor disturbance to the galaxy. The color index suggests a relatively old stellar population.
