  We present lightcurves, shapes, and a 3D convex spin-axis model for the
main-belt asteroid (2501) Lohja. The models were obtained with the lightcurve
inversion process using combined dense photometric data from the apparitions
between years 2006 and 2017. The analysis found a sidereal period of
3.80835\,hours, and a possible ecliptic pole solution (J2000.0), the prograde
sense of rotation and main ratios of the ellipsoidal model.
