The galaxy presents as a centrally concentrated, elliptical object with a smooth, diffuse morphology. There is no readily apparent disk structure or spiral arm features. The core region exhibits a bright, yellowish-white hue, suggesting an older stellar population. Progressing outwards, the color gradually fades towards the periphery, transitioning into a less intense reddish-brown hue. This suggests a potential decrease in stellar density and/or a change in stellar population with increasing radial distance from the galactic center. No significant tidal disturbances or ongoing mergers are immediately discernible. Overall, the galaxy appears to be relatively undisturbed and evolved.
