  Galactic black hole candidate Swift~J1753.5-0127 was discovered on 2005 June
30 by the Swift Burst Alert Telescope. We study the accretion flow properties
during its very first outburst through careful analysis of the evolution of the
spectral and the temporal properties using the two-component advective flow
(TCAF) paradigm. RXTE proportional counter array spectra in $2.5-25$ keV are
fitted with the current version of the TCAF model fits file to estimate
physical flow parameters, such as two component (Keplerian disk and
sub-Keplerian halo) accretion rates, properties of the Compton cloud, probable
mass of the source, etc. The source is found to be in harder (hard and
hard-intermediate) spectral states during the entire phase of the outburst with
very significant jet activity. Since in TCAF solution, the model normalization
is constant for any particular source, any requirement of significantly
different normalization to have a better fit on certain days would point to
X-ray contribution from components not taken into account in the current TCAF
model fits file. By subtracting the contribution using actual normalization, we
derive the contribution of X-rays from the jets and outflows. We study its
properties, such as its magnitude and spectra. We find that on some days, up to
about 32\% X-ray flux is emitted from the base of the jet itself.
