The galaxy presents as two distinct components. One is a centrally concentrated, relatively smooth, and roundish structure exhibiting a yellowish-orange hue. The other is a more diffuse and less concentrated bluer component which appears to be interacting or merging with the more prominent yellow component. There is no clear spiral structure apparent, but a complex interaction between the two components is likely occurring. Faint tidal features or disturbances may exist, but the resolution is insufficient for definitive confirmation. The galaxy appears to be undergoing some form of gravitational disturbance or merger.
