[2] The asteroid is orbiting at a distance of 3.39 AU from the Sun with a period of 6.24 years and an eccentricity (ovalness) of 0.26.

[1] 225 Henrietta belongs to Cybele group of asteroids and is probably in a 4:7 orbital resonance with the planet Jupiter.

[3] This is classified as a C-type asteroid and is probably composed of primitive carbonaceous material.

Photometric measurements made from the Oakley Southern Sky Observatory during 2012 gave a light curve with a period of 7.352±0.003 h and a variation in brightness of 0.18±0.02 in magnitude.

[4] In 2001, the asteroid was detected by radar from the Arecibo Observatory at a distance of 1.58 AU.