Class II methanol (CH_3_OH) masers are amongst the clearest signposts of recent high-mass star formation (HMSF). A complete catalogue outlines the distribution of star formation in the Galaxy, the number of young star-forming cores, and the physical conditions of their environment, made possible by the Global View on Star Formation (GLOSTAR) survey. This blind survey of the radio regime of 4-8GHz maps the Galactic mid-plane in the radio continuum, 6.7GHz methanol line, the 4.8 GHz formaldehyde line, and several radio recombination lines. We present an analysis of the observations of the 6.7GHz CH_3_OH maser transition using data from the D-configuration of the Very Large Array (VLA). We analysed data covering Galactic longitudes from -2{deg}