The galaxy appears to be undergoing a significant merger event. There is a primary, centrally located component that seems relatively smooth. Extending from this core is a tidal tail, exhibiting a diffuse, elongated structure. There is a secondary bright component which is most likely a second galaxy that is interacting and merging with the primary one. The overall color suggests a mixed stellar population, with redder hues concentrated in the central regions and bluer tones in the outer structures of the tidal tail. There are morphological disturbances and asymmetries present, indicative of ongoing gravitational interactions and active star formation regions, particularly along the extended tail. The light from the galaxy is relatively faint, suggesting a distant object.
