Left panel: comparison of the inclination values derived with Galfit on HST/F814W image to those obtained with GalPaK^3D on MUSE data for the spatially resolved MUSE-HDFS galaxies (red points). Right panel: comparison of the values obtained with 2D modeling to those obtained with GalPaK^3D for the disk major axis position angle for the spatially resolved MUSE-HDFS galaxies (red points). For nine galaxies (ID #5, 6, 11, 16, 17, 23, 37, and 88), the kinematical PA was constrained in GalPaK^3D to be close to the morphological PA, i.e.,  within ±10°. Labels indicate the galaxy IDs. The solid line represents the 1:1 relation and dashed lines indicate the typical scatter around this relation due to measurement uncertainties.