The galaxy appears as a centrally concentrated, smooth distribution of light. It presents an elliptical morphology with a relatively high degree of circularity. The color gradient transitions from a bright, yellowish core to a slightly redder and fainter outer halo, suggestive of an older stellar population dominating the central regions. There may be some very minor visual disturbances in the outer parts of the galaxy. No prominent spiral arm structures or significant dust lanes are discernible in this image.
