The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a high degree of roundness, lacking any distinct features such as spiral arms or a prominent disk. The color profile indicates a yellow-red hue, suggesting an older stellar population and reduced ongoing star formation. There is no visible evidence of recent mergers or major disturbances in its structure. The galaxy appears to be a relatively undisturbed, spheroidal system.
