We present a combination of high-resolution Hubble Space Telescope and wide-field ground-based and Galaxy Evolution Explorer data of the Galactic Globular Cluster M10 ( NGC6254 ) .
By using this large data-set we determined the center of gravity of the cluster and we built its density profile from star counts over its entire radial extension .
We find that the density profile is well reproduced by a single-mass King model with structural parameters c = 1.41 and r _ { c } = 41 \arcsec .
We also studied the Blue Straggler Star population and its radial distribution .
We count a total number of 120 BSS within the tidal radius .
Their radial distribution is bimodal : highly peaked in the cluster center , decreasing at intermediate distances and rising again outwards .
We discuss these results in the context of the dynamical clock scheme presented by Ferraro et al .
( 2012 ) and of recent results about the radial distribution of binary systems in this cluster .