Scaling relations for the characteristics of the abundance ratios in our sample of LINER-like galaxies. Panels in the first row show the MZR, and the continuous line represents the fit obtained by Curti et al. (2020). Panels in the second row show the MNOR, with the continuous line representing the fit obtained by Andrews & Martini (2013). Panels in the third row show the log(N/O) vs. 12+log(O/H relation), with the lines representing the different fits explained in Fig. 10. Panels in the first column show the chemical abundance ratios estimated at the effective radius. Panels in the second column show the estimations of nuclear abundances assuming AGN models with α_OX = −1.6 (abundance of the Narrow Line Region, NLR). Panels in the third column show the intersects of the metallicity radial fits. For all plots, blue dots represent galaxies with no breaks in their corresponding radial fits, green dots have one break, and red dots represent galaxies with two breaks.