The galaxy presents as a singular system comprised of what appears to be two distinct, yet gravitationally interacting, components. The overall structure is elliptical, with a dominant central bulge exhibiting a smooth, featureless morphology. The galaxy's color is generally yellow-orange suggesting a population of older stars. There is a hint of tidal disruption, manifested as a very faint extension or bridge of light connecting the two central cores, although the signal is weak, implying a potentially early stage of interaction or merger. The outer isophotes of the galaxy are elongated, with a slight deviation from perfect ellipticity.
