The galaxy appears as a singular, relatively bright object with a smooth morphology. The light distribution suggests a centrally concentrated structure, likely an elliptical galaxy. The color indices, derived from the DESI magnitudes, indicate a redder appearance, suggestive of an older stellar population. There are no visually discernible spiral arms or significant dust lanes, and no signs of recent major mergers. The overall form is somewhat circular. Based on the image and supporting data, the galaxy likely has a relatively high stellar mass, and a comparatively low star formation rate.
