The galaxy appears to be undergoing a significant merger event. The system presents with what seems to be two distinct luminous components, likely representing the interacting galactic nuclei. The primary nucleus displays a more rounded morphology, whereas the apparent secondary nucleus has a slightly more elongated appearance. There is evidence of tidal disruption and distortion, suggesting a relatively advanced stage of interaction. The overall color profile indicates a mixed stellar population with a presence of both older, redder stars and younger, bluer star formation regions. The system exhibits a relatively smooth light distribution indicating a later stage merger. The tidal features observed would indicate a system containing gas and dust, which will cause future star formation.
