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We report the results of a detailed analysis of a deep simultaneous $130\,\rmks$ \textit{XMM-Newton & NuSTAR} observation of the nearby ($z=0.0315$) andbright ($L_{\rm bol}\sim3\times10^{45}\,\rm erg\,s^{-1}$) starburst-AGNSeyfert\,2 system: MCG--03--58--007. From the broadband fitting we show thatmost of the obscuration needs to be modeled with a toroidal type reprocessorsuch as \texttt{MYTorus} \citep{MurphyYaqoob09}. Nonetheless the signature of apowerful disc-wind is still apparent at higher energies and the observed rapidshort-term X-ray spectral variability is more likely caused by a variable zoneof highly ionized fast wind rather than by a neutral clumpy medium. We alsodetect X-ray emission from larger scale gas as seen from the presence ofseveral soft narrow emission lines in the RGS, originating from a contributionof a weak star forming activity together with a dominant photoionized componentfrom the AGN.

Evidence for a clumpy disc-wind in the star forming Seyfert\,2 galaxy MCG--03--58--007