The galaxy presents as a system of two interacting galaxies. Both appear luminous in the observed bands, with a yellowish-white hue indicative of an older stellar population. The morphology suggests a possible ongoing merger, characterized by noticeable tidal disturbances and distortions in the overall structure of each galaxy. A bridge of material or tidal tail is also present between the galaxies, which is further indicative of gravitational interaction and ongoing merging activity. The shape of each galaxy in this system is distorted from a typical spiral or elliptical form, likely due to the tidal forces involved in the merger. Neither galaxy possesses a single, well-defined nucleus and instead presents with a more diffuse appearance.