 "Manto" 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 1.7–2.9 AU once every 3 years and 6 months (1,293 days; semi-major axis of 2.32 AU).Its orbit has an eccentricity of 0.27 and an inclination of 6° with respect to the ecliptic.