The galaxy presents as a centrally concentrated, elliptical-like structure. The core region exhibits a significantly higher surface brightness, displaying an orange hue, suggesting an older stellar population dominated by redder giants and dwarfs, and relatively low star formation. Moving outwards from the center, the galaxy exhibits a gradual decrease in surface brightness, transitioning to a fainter, greenish-yellow outer halo. This color suggests a mix of stellar populations, potentially including younger stars or a lower metallicity population compared to the core. The overall shape is predominantly smooth, with only subtle hints of any disk-like structure or distinct features. There is no obvious evidence of any ongoing major mergers or strong tidal interactions, although subtle disturbances cannot be entirely ruled out.
