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Based on the Galileo metadata the analytical box-wing model has been composed for theevaluation and absorption of the non-gravitational perturbing forces, i.e., SRP, albedo orEarth’s infrared radiation. The box-wing model can absorb up to 97% of the direct SRPwhereas the rest can be compensated by a set of the estimated empirical parameters. Thisstudy presents the assessment of the non-gravitational perturbing forces acting on the Galileosatellites, as well as indicates the most suitable POD strategy allowing for the determinationof the Galileo orbits with the accuracy of 25 mm in terms of SLR observation residuals.