The object presents as two spheroidal, likely elliptical galaxies in close proximity, and potentially gravitationally interacting. The larger of the two appears smooth and highly rounded. The smaller one is also smooth and rounded but with a slightly more elongated, less spherical shape. Color gradients are visible, trending from red in the outer regions towards green and yellow in the core of each galaxy. The redder hues may indicate older stellar populations in the outskirts. The brighter, yellower cores could indicate more recent star formation or a different chemical composition. A minor disturbance or a merger event cannot be ruled out, although the overall structure of both galaxies appears relatively undisturbed.
