The galaxy presents as a centrally concentrated object with a smooth, relatively featureless appearance. Its morphology appears elliptical or spheroidal, exhibiting a high degree of radial symmetry. The light distribution indicates a centrally dominant component with a gradual decrease in surface brightness outward. The galaxy's color gradient suggests older stellar populations dominate, possibly exhibiting minimal ongoing star formation. Subtle color variations might exist, but the overall impression is that of a red and relatively passive system. There's an indication of a possible minor disturbance or interaction.
