The study of globular clusters plays an important role on our understanding of the Universe since these systems are true laboratories for theories of stellar dynamics and evolution.Although the common,traditional astronomical knowledge about these systems picture them as homogeneous polytropes,made of single stellar populations,the detailed photometrical study and chemical tagging of their constituent stars suggest that some are far from being homogeneous systems.The discrepancies from the canonical picture include double(or even triple)main sequences and/or red giant branches,larger than expected internal chemical abundance scatter and unusual horizontal branch showing simultaneously extremely blue and red stars.Some of these non-canonical clusters are now being seen as remmants of the nuclei of former satellite galaxies of the Milky Way.A similar awkward extragallactic globular cluster(Scl-dE1 GC1)in the Sculptor Group dwarf elliptical galaxy Scl-dE1(Sc22),studied by Da Costa et al.has a half-light radius of 21.8 pc,an absolute magnitude of MV=-6.7 and the cluster stellar population appears indistinguishable from that of the parent galaxy.Da Costa et.al suggest that this object might have formed through the merging of star clusters.This scenario for the formation of Scl-dE1 GC1 was succesfully reproduced by Assmann et al.with a particle-mesh code.Since the globular cluster configuration correspond to a relatively small,relaxed gass-free stellar system supported by velocity dispersion,it is likely that a number of different objects,by means of their formation path,could end up as globular-like systems,including some globulars formed by early collisions of other globulars.We here study the outcomes of collisions between globular clusters under the gravitational influence of a larger disk galaxy.We use the NBODY6 direct N-body code by Aarseth to check under which conditions a close encounter of two globulars could disrupt them or lead to a merged,larger globular.We check whether merged globulars have a peculiar luminosity profile right after the merger and how much time it takes for a new relaxation.