Best-fit kinematics for the single stellar component model. The two-dimensional maps show the velocity and velocity dispersion fields. The plots on the side show some example of reconstructed non-parametric LOSVDs in the location of the field of view indicated by the dotted lines. The LOSVDs of central regions clearly show a bimodal distribution; the LOSVDs in the outer regions show high asymmetry, which can be due to the presence of an unresolved secondary kinematic component.