The galaxy appears as a single, relatively smooth, centrally concentrated object. Its overall shape is largely elliptical and round. The galaxy exhibits a color gradient, transitioning from a yellowish core to redder hues in its outer regions. No distinct spiral arms, bars, or other prominent features typically associated with disk galaxies are visible. There are no signs of any major or minor mergers occurring with other galaxies. The galaxy is dominated by an older stellar population as indicated by its color. There is a small amount of on going star formation activity. Based on its estimated distance, its physical size is a few kpc across. The estimated mass is around 10^10 solar masses.
