Results of UMSCANGALACTIK applied to all kinematic map types of our galaxy sample at different inclinations. Top panels: HDBSCAN clusters in UMAP bidimensional projection of the set of all kinematic maps of galaxies observed at 60, 45, and 30 degrees. The outliers of the method are shown as grey dots. Middle panels: UMAP projection obtained from all kinematic map types according to the clustering obtained for the line-of-sight velocity maps discussed in Sect. 4, colour-coded as in Fig. 5Bottom panels: Distributions of D/T on each projection. The colour bar limits are fixed to the 10th and 90th percentiles of the variables.