The object presents as an elliptical galaxy with a relatively smooth morphology. The central region exhibits a concentrated luminosity, appearing as a bright, slightly reddish core. Moving outward from the center, the light gradually diminishes. While generally smooth, there is a hint of a disk-like structure, with a subtle flattening observed. Overall, the galaxy appears to be in a relatively stable and unperturbed state, with no major signs of mergers or significant tidal disturbances. A slight color gradient is observable, transitioning from a redder core to bluer outer regions. This could indicate a population of older stars concentrated in the galactic center and younger stars in the outer regions.
