The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a concentrated, bright golden hue, suggestive of an older stellar population. A subtle color gradient is observed, transitioning from the yellowish core to a more diffuse, red-tinged outer region. The isophotes appear regular and concentric, and exhibit an high axial ratio of ~0.9. There is no obvious presence of spiral arms or distinct dust lanes. Overall, the galaxy gives an impression of being a relaxed system.