The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a higher concentration of light, appearing yellowish-orange, suggesting an older stellar population. Moving outwards from the core, the light gradually diminishes in intensity. The outer regions display a hint of a flattened disk, with a subtle greenish hue that may indicate the presence of some younger, star-forming regions, although these appear minimal. Overall, the galaxy seems relatively undisturbed with no apparent major mergers or tidal features. The overall shape suggests a classification somewhere between a lenticular and elliptical galaxy.
