The energy difference is small near major-shell closures but large in the middle of the major shells. Apart from this shell fluctuation, one can see some overall trends. For each of the three major shells of neutrons divided by N=50, 82, 126, and 184, the largest energy difference is 4.70 MeV (124Sm, delta=-0.25, 0.37), 6.58 MeV (164Gd, delta=-0.22, 0.31), and 11.05 MeV (254No, delta=-0.17, 0.26), respectively; as the nucleus becomes heavier, the energy difference increases while the size of deformation decreases. For nuclei with N < 50, the changes along isotope chains are not so regular as in heavier nuclei and the oblate solutions often have lower energies than prolate ones. For nuclei with N > 50, oblate ground states are very rare and found only in nuclei very close to shell magics. The dominance of prolate deformations for N >50 may be attributed to the change of the nature of the major shells from the harmonic-oscillator shell to the Mayer-Jensen shell.