 "Seraphina" 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 outer asteroid belt at a distance of 2.5–3.3 AU once every 4 years and 11 months (1,802 days; semi-major axis of 2.9 AU).Its orbit has an eccentricity of 0.13 and an inclination of 10° with respect to the ecliptic.