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We have recently reported on the discovery of a new X-ray variability pattern from the nucleus of the galaxy GSNvirgul069 comma dubbed as Quasi-Periodic Eruptions comma or QPEs openParMiniutti et al. 2019 comma Nature comma 573 comma 381closePar. We propose here for further XMM-Newton observations to better characterize this newly-discovered variability pattern. Ideally comma our observations will be complemented with 2 HST orbits with the goals ofdoublePoint iclosePar deriving the optical to X-ray SED of GSNvirgul069 iiclosePar search for possible blue point sources other than the galactic nucleus in comparison with our Chandra data iiiclosePar study the morphology of the poorly known host galaxy ivclosePar study the spatially-resolved structure of the narrow-line-region in CORCHETE_OPENOvirgulIIICORCHETE_CLOSE.