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Fitting with standard models, we find that both sources show similar spectra characterized by a heavy absorption with $N_{\\rm{H}} \\simeq 10^{24} \\ \\rm{cm}^{-2}$, the fraction of scattered light is $f_{\\rm{scat}} = 0.5-0.8%$, and the solid angle of the reflection component is $\\Omega/2\\pi = 0.4-1.1$. To investigate the geometry of the torus, we apply numerical spectral models utilizing Monte Carlo simulations by Ikeda et al. (2009) to the Suzaku spectra. 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