Flux maps created from the results of the spaxel-by-spaxel multi-Gaussian fitting. Upper row: the flux of the Hα and [N II]λ6584 Å narrow components representing the host galaxy emission from left to right, respectively. Bottom left panel: the flux of the outflow component traced by the [N II]λ6584 Å broader component. Bottom right panel: the broad Hα component that traces the emission from the BLR. The x and y axes are the displacement in arcseconds from the galaxy center at RA = 03:32:29.3, Dec = −27:56:19.6.