The galaxy appears as a centrally concentrated object with a smooth, symmetrical morphology. Its light profile suggests a relatively uniform distribution, characteristic of an elliptical galaxy. There is a slight color gradient visible, transitioning from a warmer, redder hue near the core to a cooler, bluer hue further out, indicating older stellar populations concentrated in the center. No distinct spiral arms or other features are evident. The galaxy is not undergoing any major mergers or intense star formation.