Shape model for 495 Eulalia reconstructed from the available lightcurves for the pole P1 solution. Left and middle parts yield two perpendicular equatorial views, right panel shows a view from the rotation pole. The majority of non-calibrated data constrain principally the equatorial axes ratio (which is small in this case because lightcurve amplitude never exceeds 0.5 mag). The polar stretching-factor is less constrained with the present dataset, but our tests indicate the asteroid is not near-spherical.