MUSE NFM surface brightness map of the Hα emission. The black contours show the S/N levels of the Hα emission of 3, 5, and 10. The gray contours show the morphology of the blueshifted CO (3–2) molecular outflow (B19), at the emission levels of 1, 4, 8, and 10 mJy. The black circles indicate regions affected by significant residuals in the PSF subtraction due to the quasar and a nearby continuum source.