The galaxy presents as a primarily smooth, elliptical-like structure with a high degree of central concentration. The core region exhibits a bright, yellowish-white hue, indicative of an older stellar population likely dominated by red giant stars. The surrounding halo gradually fades in intensity, showing a smoother, more diffuse distribution of light, with subtle color gradients suggesting variations in stellar population or dust content. There is a subtle hint of a disk-like structure, however the smoothness of the light profile dominates. Minor disturbances or asymmetries are not immediately apparent, although higher resolution data might reveal faint tidal features or evidence of past interactions. Overall, the galaxy appears relatively undisturbed and relaxed in its morphology, suggestive of an evolved system with potentially low current star formation activity. The galaxy appears moderately massive with estimates indicating a mass over 10^10 solar masses.
