Flux (left panel), velocity (middle panel), and velocity dispersion (right panel) maps for the stellar component of SDSS1524+08. Overplotted in gray are the ellipses fitted to the isophotal profiles. This fit indicates a close-to-face-on disk. Outside the main centrally-concentrated stellar distribution, there are clear tidal tails that dominate the stellar distribution. The velocity map indicates little to no sign of rotation, with an apparent small gradient in velocity in the central region. The velocity dispersion map shows a high velocity dispersion in the redshifted region NE of the nucleus and seemingly along the tidal tail that goes E to N. This indicates very low rotational support in the stellar distribution.