The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is a distinct core that is much brighter than its surrounding halo, suggesting a high concentration of stars. The central region exhibits a yellowish-white color, indicative of an older stellar population. The outer regions are fainter and show a slight blueish tinge, perhaps hinting at ongoing, but minor star formation. No obvious spiral arms or disk structures are visible. The galaxy exhibits a near circular shape. There are no signs of significant tidal disturbances or ongoing mergers that are readily apparent.