We have observed the nucleus of NGC2110 (a Seyfert S0 galaxy with a radio jet) with the Keck OSIRIS instrument (using AO) across the infrared in the J, H and Z bands, with a resolution of 5 pc per pixel. The circumnuclear torus is resolved into a number of luminous star clusters, which are each comparable to the mass and luminosity of the Arches Cluster at the centre of the Milky Way.