UBVI and $H{alpha}$ CCD photometry of IC 1848, one of active star-forming regions in Cas OB6, is carried out as a part of Sejong Open cluster Survey (SOS) project. An OB association is an ideal laboratory for studying the triggered star formation and star formation history. Our purposes are to provide deep photometric data up to 21 mag in V and physical parameters of IC 1848. We classify 79 early-type stars and 186 pre-main sequence (PMS) stars as being the members of the cluster using photometric criteria. The IR excess emission PMS stars by Koenig et al. (2008) are also included as members of IC 1848. Total number of members is 414. We derive the interstellar reddening (<E(B-V)>=$0.659{pm}0.058$ mag), reddening law ($R_V=4.0{pm}0.1$), distance modulus ($V_0-M_V=12.0{pm}0.1$ mag) using the early-type members of IC 1848. We also determine the age of the cluster ($3.5{pm}1.5$ Myr) by placing the theoretical isochrones on the HR diagram.