 "Hooveria" is a non-family asteroid of the main belt's background population when applying the hierarchical clustering method to its proper orbital elements.It orbits the Sun in the inner asteroid belt at a distance of 2.2–2.6 AU once every 3 years and 9 months (1,375 days; semi-major axis of 2.42 AU).Its orbit has an eccentricity of 0.09 and an inclination of 8° with respect to the ecliptic.