[O III] (top) and Hα (bottom) flux, moment-1 and moment-2 maps for the outflow kinematic component. A S/N cut of 4 has been applied to generate the maps. The [O III] maps show a typical biconical outflow structure, oriented along the NE-SW direction, consistent with our spectro-astrometry analysis (Sect. 4.1). The Hα flux distribution is less extended, as this Balmer line is fainter than [O III].