We present the Suzaku results on a new candidate of a supernova remnant (SNR) in the Sagittarius C region. We detected diffuse X-rays of an elliptical shape (G 359.41-0.12) and chimney-like structure (the Chimney), both of which are fitted with a thin thermal model of KT 1 keV temperature. The absorption columns are same between these two structures, indicating the both are located at the same distance in the same line of sight. The narrow band image and one-dimensional profile of S-XV K alpha at 2.45 keV show that the Chimney is emanating from G 359.41-0.12. Therefore these two sources are physically connected with each other. The sum of thermal energies of the Chimney and G 359.41-0.12 is estimated to be 1.4* 1050 ergs, typical for a Galactic SNR. G 359.41-0.12 is likely a new SNR candidate and the Chimney is an associated outflow.