Arp102B is a nearby radio galaxy which displays the presence of double peaked Balmer emission lines .
Sub-arcsec Keck mid-infrared imaging and Spitzer spectroscopy reveal a spatially compact mid-infrared source which displays tentative evidence for variability .
The F _ { \nu } \propto \nu ^ { -1.2 } spectral energy distribution is suggestive of an advection dominated accretion flow .
The absence of dust features over the 5 - 40 \mu m range make it unlikely that thermal dust emission dominates the mid-infrared luminosity .
We also detect the presence of molecular hydrogen in emission which is asymmetrically redshifted by \sim 500-1000 km/s from the systemic velocity of the galaxy .
Since the forbidden , low ionization lines in this galaxy are at the systemic velocity , we suggest that the molecular hydrogen emission arises from a rotating molecular gas structure surrounding the nuclear black hole at a distance of \sim 1 pc .