The galaxy presents as a relatively compact object. Its morphology appears to be generally smooth and elliptical, with a high degree of central concentration. The light distribution suggests it is predominantly spheroid in shape. The galaxy is located at a considerable distance, as evidenced by its redshift. The galaxy's color indices suggest it's composed predominantly of an older stellar population, showing redder colors. There is no distinct presence of any spiral arms or features. There is no strong evidence of current, ongoing major mergers or interactions; however, some minor asymmetry may suggest some past disturbance.
