structure toward the central part of the filamentary feature. The infrared shell is spatially located inside this temperature structure, and is traced in a temperature range of about 20–26.5 K. Furthermore, a cold region (T$_{d}$ $\sim$13.5–15 K) inside the temperature structure is also found in the [*Herschel*]{} temperature map. As mentioned earlier, the signatures of outflow activities are mainly found toward the IRDCs, where higher column density materials are observed in the [*Herschel*]{} column density map. Using the column density map and the [*clumpfind*]{} algorithm [@williams94], we have identified twenty three clumps in our selected target site, and have also computed thier physical parameters (i.e., mass (M$_{clump}$), radius (R$_{clump}$), and average volume density ($n_{\mathrm H_2}$)). To find the clumps, we provided several column density contour levels (i.e., (3.9, 5.0, 6.0, 7.0) $\times$ 10$^{21}$ cm$^{-2}$) as an input parameter for the [*clumpfind*]{}, where the lowest contour level was chosen at about 6$\sigma$. In Figure \[fig2\]c, the boundaries of these clumps are shown along with their labels. The values of M$_{clump}$, R$_{clump}$, and $n_{\mathrm H_2}$ of each [*Herschel*]{} clump are listed in Table \[tab1\]. Here, the average volume density ($n_{\mathrm H_2}$ = 3M$_{clump}$/(4$\pi$R$_{clump}^{3}$$\mu_{H_2} m_H$)) of each clump is estimated using the values 