The galaxy appears as a luminous, elliptical object with a smooth, centrally concentrated light profile. The core exhibits a bright, yellowish-white hue, suggesting a population of older stars. The outer regions show a gradual decrease in luminosity, transitioning to a more reddish-orange color. There is no visible dust lane, spiral arm structure, or other signs of active star formation regions. The overall morphology indicates a relatively evolved system, likely a massive elliptical galaxy. There is no evidence of recent or ongoing merger activity or significant tidal disturbances. The galaxy presents a symmetrical, well-defined shape, indicating a dynamically relaxed state.
