The galaxy presents as an elliptical morphology with a smooth, concentrated light profile. It exhibits a relatively high degree of symmetry. The color is a mixture of light blues and yellows, suggesting an older stellar population with a lower ongoing star formation rate. There is an overall lack of prominent features such as spiral arms or dust lanes. The galaxy is likely a relatively massive system at a distance of a few hundred megaparsecs. No signs of recent major merger activity are visible.
