Weights for the FMD model of NGC 3311 as a function of the radius within the MUSE fields. The four main components of NGC 3311, A, B, C, and D, are shown individually. The component A + B indicates the sum of the first two components, which are modeled as having the same kinematics. The component E−J indicates the cumulative contribution of all other photometric components that are not included in the kinematic modeling.