Using archival {it Chandra} observations with a total effective exposure of 323 ks, we derive an updated catalog of point sources in the bulge globular cluster M28. The catalog contains 502 X-ray sources within an area of $sim475, rm arcmin^{2}$, and more than $90%$ of these sources are first detected in this cluster. We find significant dips in the radial distribution profiles of X-ray sources in M28, with the projected distance and width of the distribution dip for bright ($L_{X} gtrsim 4.5times 10^{30} {rm erg ,s^{-1}}$) X-ray sources are larger than the faint ($L_{X} lesssim 4.5times 10^{30} {rm erg ,s^{-1}}$) sources. The generalized King model fitting give a slightly larger average mass for the bright sources ($1.30pm0.15,M_{odot}$) than the faint sources ($1.09pm0.14,M_{odot}$), which support a universal mass segregation delay between heavy objects in GCs. Compared with 47 Tuc and Terzan 5, we show that the dynamical age of M28 is comparable to Terzan 5 and much smaller than 47 Tuc, but it is evolving more fast (i.e., with smaller two-body relaxation timescale) than 47 Tuc. These features may suggest an acceleration effect of cluster dynamical evolution by tidal shock in M28. Besides, we find an abnormal deficiency of X-ray sources in the central region ($R lesssim 1.5 rm~arcmin$) of M28 than its outskirts, which indicate that M28 may have suffered an early phase of primordial binary disruption within its central region, and mass segregation effect will erase such a phenomenon as cluster evolve to older dynamical age.
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