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Starting with the fractal inspired distribution functions for Maxwell-Boltzmann, Bose-Einstein and Fermi systems, as reported by F. B"{u}y"{u}kkili\c{c} and D. Demirhan, we obtain the corresponding probability distributions and study their thermodynamic behavior. We compare our results with those corresponding to ideal gases (q=1), and Bose-Einstein and Fermi systems with quantum group symmetry. In particular, we show that the hamiltonian that gives the Bose-Einstein generalized distribution function can be interpreted as a q-deformation of the ideal gas hamiltonian.

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