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We present results of the Galactic supernova remnant (SNR) G355.6-0.0observed with Suzaku. We resolved the diffuse emission detected with ASCA intotwo objects, G355.6-0.0 and a point-like source, Suzaku J173530-3236. The X-rayemission from G355.6-0.0 exhibits a center-filled morphology within the radioshell. The X-ray spectrum is well represented by a thin thermal plasma modelwith enhanced metal abundances. The spatial and spectral properties imply thatG355.6-0.0 is a member of the mixed-morphology SNRs. The NH value of ~ 6 x10^{22} cm^{-2} supports that G355.6-0.0 is a distant SNR. Suzaku J173530-3236exhibits a hard X-ray spectrum with a strong Fe emission line, similar to thoseof cataclysmic variables. The NH value of ~ 3 x 10^{22} cm^{-2} is smaller thanthat of G355.6-0.0, and hence Suzaku J173530-3236 is located at the near sideof G355.6-0.0.

X-Ray Observation of the Galactic Supernova Remnant G355.6-0.0 with Suzaku