The galaxy presents as a flattened, elliptical morphology with a smooth light distribution. A central bulge is apparent, exhibiting a concentration of luminosity towards the core. The overall color suggests a mature stellar population with a relatively low rate of current star formation. There are no distinct spiral arms or obvious signs of recent mergers or major disturbances. The galaxy exhibits a disk-like structure that is tilted with respect to our line of sight. There is no indication of prominent dust lanes or significant substructure within the galaxy's visible components.
