The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. Its light profile appears relatively uniform, lacking prominent spiral arms or distinct features typically associated with disk galaxies. The core exhibits a bright, yellowish-orange hue, suggesting a population of older stars. The outer regions gradually fade into a more diffuse, reddish glow. There's a hint of bluer light mixed in with the redder outer regions, potentially indicating a small amount of recent star formation. The galaxy appears largely undisturbed, with no obvious signs of recent major merger activity or tidal distortions.
