  In the context of a project aimed at characterizing the dynamical evolution
of old globular clusters in the Large Magellanic Cloud, we have secured deep
HST/WFC3 images of the massive cluster NGC 1835. In the field of view of the
acquired images, at a projected angular separation of approximately 2 arcmin
from the cluster, we detected the small stellar system KMK88-10. The
observations provided the deepest color-magnitude diagram ever obtained for
this cluster, revealing that it hosts a young stellar population with an age of
600-1000 Myr. The cluster surface brightness profile is nicely reproduced by a
King model with a core radius rc = 4 arcsec (0.97 pc), an half-mass radius rhm
= 12 arcsec (2.9 pc), and a concentration parameter c~1.3 corresponding to a
truncation radius rt~81 arcsec (19.5 pc). We also derived its integrated
absolute magnitude (MV=-0.71) and total mass (M~80-160 Msun). The most
intriguing feature emerging from this analysis is that KMK88-10 presents a
structure elongated in the direction of NGC 1835, with an intracluster
over-density that suggests the presence of a tidal bridge between the two
systems. If confirmed, this would be the first evidence of a tidal capture of a
small star cluster by a massive globular.
