GRB 130702A is a nearby long-duration gamma-ray burst ( LGRB ) discovered by the Fermi satellite whose associated afterglow was detected by the Palomar Transient Factory . Subsequent photometric and spectroscopic monitoring has identified a coincident broad-lined Type Ic supernova ( SN ) , and nebular emission detected near the explosion site is consistent with a redshift of z = 0.145 . The SN-GRB exploded at an offset of \sim 7.6 ^ { \prime \prime } from the center of an inclined r = 18.1 mag red disk-dominated galaxy , and \sim 0.6 ^ { \prime \prime } from the center of a much fainter r = 23 mag object . We obtained Keck-II DEIMOS spectra of the two objects and find a 2 \sigma upper limit on their line-of-sight velocity offset of \lesssim 60 km s ^ { -1 } . If we calculate the inclination angle of the massive red galaxy from its axis ratio and assume that its light is dominated by a very thin disk , the explosion would have a \sim 60 kpc central offset , or \sim 9 times the galaxy ’ s half-light radius . A significant bulge or a thicker disk would imply a higher inclination angle and greater central offset . The substantial offset suggests that the faint source is a separate , dwarf galaxy . The star-formation rate of the dwarf galaxy is \sim 0.05 M _ { \odot } yr ^ { -1 } , and we place an upper limit on its oxygen abundance of 12 + log ( O/H ) < 8.16 dex . The identification of an LGRB in a dwarf satellite of a massive , metal-rich primary galaxy suggests that recent detections of LGRBs spatially coincident with metal-rich galaxies may be , in some cases , superpositions .