The galaxy presents as a centrally concentrated, relatively smooth object. It appears highly rounded, with a minimal discernible disk structure. There are no clear signs of spiral arms or a central bar. The galaxy exhibits a color gradient, appearing bluer in the core and gradually becoming redder towards the outer regions. This suggests a declining rate of star formation from the center outwards. The overall morphology indicates it is likely an elliptical galaxy. There is no significant morphological disturbance suggesting this galaxy is the product of recent galaxy mergers.
