Spectrum extracted using a circular aperture of radius $0\stackrel{″}{.}41$ from the continuum peak. The jet emission is identified in the FELs of [Fe II], and in Br-γ emission. The outflow is detected in the H₂ emission lines. In addition, CO overtone bandhead emission at 2.29−2.36 μm, which traces the inner gaseous disc, is also seen. A characteristic reddening slope is evident in this spectrum as expected, as the source is heavily extincted and only visible at infrared wavelengths. Stellar absorption lines were not identified in this spectrum, it was concluded that the central source is too heavily extincted to study these lines.