Kinematic maps for the ionized component as traced by the Hα line. From left to right, top to bottom: Flux intensity, velocity field and (intrinsic) velocity dispersion maps of the primary (systemic), secondary and tertiary components. The velocity maps of each component have been corrected for the systemic velocity, v_sys, derived at the AGN position (i.e., at the continuum intensity peak, marked by a black cross in all the maps). Gray contours in the flux intensity systemic maps trace the R-band continuum emission, highlighting the position of the foreground star. The magenta circles in the primary and secondary maps mark two individual spaxels in the northeast (NE) and southwest (SW) directions within the butterfly region, from which the spectra shown in the bottom panel are extracted. The spectra are fit with two components, and the broad [NII] emission is detected at S/N > 4 (i.e., 5.5 in the NE and 4.1 in the SW). The light gray circle in the bottom-left panel is the MEGARA PSF (FWHM). For all the maps, north is up and east to the left.