The galaxy appears as a luminous, elliptical object. Its morphology suggests it is relatively smooth with a high degree of central concentration. The galaxy exhibits a predominantly yellow-orange hue, indicative of an older stellar population and minimal ongoing star formation. The overall roundness suggests it is not a highly inclined disk galaxy, and there is no visual evidence of any major disturbances or ongoing mergers. The light is centrally concentrated, fading gradually toward the edges. No spiral arms or distinct features are visible.
