Profiles of the anisotropy parameter obtained with the Schwarzschild modeling of two stellar populations of the simulated galaxy. In rows: results for all stars (calculated as the superposition of two populations), population I, and population II. Colors follow the convention used in previous figures. In columns: observations along the major, intermediate, and minor axis. The last narrower column shows the data (black lines) outside the modeled radial range. Color lines indicate values for the best-fit models whereas the colored areas of decreasing intensity show the 1, 2, and 3σ confidence regions.