  We present a multiwavelength study of the massive star forming region
associated with IRAS 06055+2039 which reveals an interesting scenario of this
complex where regions are at different stages of evolution of star formation.
Narrow band near-infrared (NIR) observations were carried out with UKIRT-UFTI
in molecular hydrogen and Br$\gamma$ lines to trace the shocked and ionized
gases respectively. We have used 2MASS $J H K_{s}$ data to study the nature of
the embedded cluster associated with IRAS 06055+2039. We obtain a power-law
slope of 0.43$\pm$0.09 for the $K_{s}$-band Luminosity Function (KLF) which is
in good agreement with other young embedded clusters. We estimate an age of 2
-- 3 Myr for this cluster. The radio emission from the ionized gas has been
mapped at 610 and 1280 MHz using the Giant Metrewave Radio Telescope (GMRT),
India. Apart from the diffuse emission, the high resolution 1280 MHz map also
shows the presence of several discrete sources which possibly represent high
density clumps. The morphology of shocked molecular hydrogen forms an arc
towards the N-E of the central IRAS point source and envelopes the radio
emission. Submillimetre emission using JCMT-SCUBA show the presence of a dense
cloud core which is probably at an earlier evolutionary stage compared to the
ionized region with shocked molecular gas lying in between the two. Emission
from warm dust and the Unidentified Infrared Bands (UIBs) have been estimated
using the mid-infrared (8 -- 21 $\mu$m) data from the MSX survey. From the
submillimetre emission at 450 and 850 $\mu$m the total mass of the cloud is
estimated to be $\sim$ 7000 -- 9000 $\rm M_{\odot}$.
