The galaxy presents as a centrally concentrated, relatively smooth object with a roughly elliptical morphology. The core region exhibits a bright, yellowish-white hue, suggesting an older stellar population. This central luminosity decreases radially outwards into a more diffuse, greenish-blue halo. The halo appears smooth, lacking distinct spiral arms or other prominent features. The overall structure indicates a minimal amount of recent star formation and no signs of ongoing or recent merger activity based on the morphology. The light profile is smooth and fairly well-defined. 
