We report the discovery based on GLIMPSE data of a proto-stellar system driving a bipolar outflow . The bipolar outflow closely resembles the shape of an hourglass in the infrared . The total luminosity of L _ { total } = 5507 L _ { \odot } , derived from IRAS fluxes , indicates the ongoing formation of a massive star in this region . The spectral energy distribution ( SED ) of the driving source is fitted with an online SED fitting tool , which results in a spectral index of about 1.2 . This , along with the presence of a bipolar outflow , suggests the detection of a Class I protostar . The driving source indicates prominent infrared excesses in color-color diagrams based on archived 2MASS and GLIMPSE data , which is in line with an early evolutionary stage of the system .