The object presents as a galaxy with an elliptical morphology. It exhibits a smooth, concentrated light profile, suggesting an older stellar population. The galaxy appears more rounded than elongated, displaying minimal visible features such as spiral arms or a prominent disk. There is no apparent major disruption of its structure, indicating no recent major merger events. A subtle hint of disturbance may be present within the galaxy. The overall color is predominantly yellow-orange, possibly indicating lower ongoing star formation. The galaxy is of intermediate size, but its high luminosity means it is a massive galaxy at a significant distance.
