The galaxy presents as a singular, unresolved luminous entity. It appears elliptical or possibly lenticular, exhibiting a smooth, rounded morphology with no discernible spiral arm structure or prominent disk features. The light distribution is centrally concentrated with a gradual decrease in intensity outward from the core. The color profile suggests a population of older stars, potentially with limited recent star formation. There is no evidence of any major ongoing merger activity or significant tidal disturbances affecting the galaxy's overall form. The galaxy is of considerable size and mass, exhibiting high luminosity.
