The galaxy presents as a diffuse, elliptical structure with a smooth, centrally concentrated light distribution. A subtle blue tint is visible, suggesting the presence of younger stars. The galaxy's shape appears to be somewhere in between round and elliptical. There are faint signs of minor disturbances within the galactic structure. These disturbances could be the result of a minor merger event or some other gravitational interaction. No strong evidence of spiral arms or a prominent disk is discernible.