The galaxy exhibits an elliptical morphology with a smooth light distribution. The central bulge region is bright, and a subtle disk component appears present. The galaxy's shape is somewhere in between round and elongated. There are no major disturbances visible suggesting there are no ongoing mergers. The galaxy possesses a redder hue which may be due to an older stellar population and/or dust content. Overall, the galaxy appears to be a relatively massive system, undergoing a low rate of star formation.
