  The Galactic supernova remnant (SNR) MSH 15-56 is a member of the class of
composite SNRs that consists of the remnant shell and a displaced pulsar wind
nebula (PWN). The earlier X-ray observations reported the comet-like morphology
of the PWN and the ejecta distribution of the SNR. In this work, we present a
study of MSH 15-56 using archival Suzaku data. We investigate the nature of the
emission and spectral parameters of the remnant. The X-ray spectra are well
fitted with a combination of a thermal and non-thermal model with temperature
~0.6 keV and photon index ~2.0. The slightly enhanced abundances of Ne, Mg, S
and enhanced abundance of Si confirm the presence of ejected material.
