The deposit type on the Lara Property is classified as Kuroko-type massive sulphides comprising volcanic-hosted, stratiform accumulations of sphalerite, pyrite, chalcopyrite, galena and tetrahedrite.It is the most significant VMS deposit outside of the Mt. Sicker deposits in the area and occurs at shallow depths of <150 m below surface. Previous metallurgical testing and pre-feasibility studies (Roberts, 2007; Broughton, 1987) although not current, demonstrate the possibility that the deposit could be economic and deserves further investigation. Furthermore, there is abundant exploration potential to depth and along strike along the Coronation Trend to warrant additional exploration as VMS deposits such of these tend to occur as clusters including the most immediate analogues (Mt. Sicker and Buttle Lake Myra Falls deposits). Proximity to former producing mines may not be indicative of the potential of the Lara Project.