Smooth histograms of multiple host galaxy properties. Top (left to right): b/a axis ratio, log(M_⋆), and log(SFR) from Pipe3D. Bottom (left and middle plot): log(L_{[O III]}) and log(EW(H_α)), both extracted from an aperture of 1 R_eff, and (to the right) a complementary illustration for Table 2 employing Venn diagrams. In order to maintain visual clarity, the hard X-ray-selected AGN sample was intentionally omitted from the diagrams. The gray-shaded histogram shows the distribution of all MaNGA that pass our S/N criteria (see Sect. 3.2).