Dust attenuation (a) and line ratio maps (b), (c) constructed based on the fit fluxes integrated for all components. The white and gray contours indicate the 5σ and 15σ [O III] surface brightness levels of the un-smoothed systemic narrowband image, respectively (Fig. 1). Dark purple lines show the directions toward the radio jet hot spots. Black triangle marks the position of the AGN while magenta contours trace the ALMA continuum (Fig. 1d). The dashed white lines and circle in panel b and c divide the FoV into five regions for line ratio diagnostic analysis (Fig. 5). FWHM of the JWST PSF is marked at the left corner.