The observed galaxy presents a distinct morphology suggesting an ongoing or recent merger event. There is a disturbed structure, with an asymmetry in the main body of the galaxy. Evident distortions hint at gravitational interactions. There is evidence of a faint tidal tail extending outwards. The central region appears moderately smooth, while the outer regions display a clumpy, disturbed texture. The colour profile appears relatively uniform across the galaxy, with slight variations that may indicate differing stellar populations or dust distribution as a result of the merger. The object's apparent size is relatively small.
