The galaxy presents as a centrally concentrated, roughly circular object. Its light profile appears smooth and diffuse, indicating a lack of prominent spiral arms or distinct structural features. The color gradient transitions from a yellowish core to a slightly redder outer region. This suggests an older stellar population is more dominant throughout the galaxy. There's no evidence of significant dust lanes or active star-forming regions. Overall, the galaxy appears morphologically relaxed, consistent with an elliptical or lenticular type. There are no signs of any recent or ongoing merger activity.
