  We report the discovery of emerged tidal tails around open cluster IC 4756
($\sim$ 1 Gyr) based on 644 members identified from {\it Gaia} EDR3.
Three-dimensional spatial positions, two-dimensional tangential velocities
$\left( x, y, z, \kappa \cdot \mu_{\alpha}^{*}/\varpi, \kappa \cdot
\mu_{\delta}/\varpi \right)$ are utilized to determine the co-moving member
candidates of IC 4756. Using a Bayesian method, we correct the distance for
each cluster member. Two tidal tails extend up to 180 pc and display a S-shape
in $X^{\prime}Y^{\prime}$ space (Cartesian coordinates focused on cluster
center). A clean sequence of our members in Color-Absolute-Magnitude Diagram
(CAMD) indicates the coeval population and matches perfectly with the PARSEC
isochrone with age from Bossini et al. (2019). Mass segregation is detected in
this cluster as well. Finally, we derive the tidal radius and core radius of IC
4756 about $12.13$ pc and $4.33 \pm 0.75$ pc, respectively.
