Ionized gas maps as derived from the Hα emission line profiles. First row: the equivalent width map, velocity field, and velocity dispersion map of the main (narrow) Hα component. Second row: the same as the first row but for the secondary (broad) component. EWs maps are in Å, while the kinematic maps are in km s^-1. We note that these maps have been zoomed-in for consistency with the NaD maps. The cross marks the galaxy nucleus, as in Fig. 4. The black dashed boxes in the velocity map (narrow component) mark the regions where the integrated spectra are obtained and analyzed (see Sect. 4.4).