Comparison of the pseudo-narrowband images convolved with a Gaussian of 1″ FWHM, computed for the MUSE data cube (left) and the best-fitting model cube (center), collapsing the Mg II wavelength range, after subtracting the continuum from both cubes, for the full modeled FoV. The residuals are shown in the right panel. The magenta cross indicates the center of the FoV for reference. There is a good qualitative agreement between the images, with each displaying an absorption-dominated center, shown in red, and a more spatially extended halo of emission Mg II emission, shown in gray colors. However, there are also clear differences in the morphology and strength of the Mg II emission.