Non-parametric recovery of the stellar LOSVD. We show the recovered LOSVD derived from the spectral binning in each spaxel of the MaNGA spectrum using Gaussian fitting techniques. The number of Gaussian components fitted varies according to the spatial location of each spaxel. Initially, all spaxels were fitted with a Gaussian representing the a₁ component (in blue). Additional Gaussian components were incorporated in regions where extra kinematic structures were identified (denoted by circles a₂, b, and c, and coded in orange, green, and red). The merged spaxels used for the two-component full-spectrum fitting are shown as highlighted regions in the corresponding colours. Within these regions, vertical lines mark the velocities obtained from the full-spectrum fitting procedure, which are consistent with the two-Gaussian fits of the recovered non-parametric LOSVDs.