We present results for an up-to-date uncatalogued star cluster projected towards the Eastern side of the Large Magellanic Cloud ( LMC ) outer disc .
The new object was discovered from a search of loose star cluster in the Magellanic Clouds ’ ( MCs ) outskirts using kernel density estimators on Washington CT _ { 1 } deep images .
Contrarily to what would be commonly expected , the star cluster resulted to be a young object ( log ( t yr ^ { -1 } ) = 8.45 ) with a slightly subsolar metal content ( Z = 0.013 ) and a total mass of 650 M _ { \odot } .
Its core , half-mass and tidal radii also are within the frequent values of LMC star clusters .
However , the new star cluster is placed at the Small Magellanic Cloud distance and at 11.3 kpc from the LMC centre .
We speculate with the possibility that it was born in the inner body of the LMC and soon after expeled into the intergalactic space during the recent Milky Way/MCs interaction .
Nevertheless , radial velocity and chemical abundance measurements are needed to further understand its origin , as well as extensive search for loose star cluster in order to constrain the effectiveness of star cluster scattering during galaxy interactions .