 According to Zappalà's classification of dynamical families, and when applying the synthetic hierarchical clustering method (HCM) by Nesvorný, "Kovacia" is a member of the Hygiea family (), a very large family of carbonaceous outer-belt asteroids, named after 10 Hygiea, which is the main belt's fourth-largest asteroid.However, it is a non-family background asteroid according to another HCM-analysis by Milani and Knežević (AstDys).It orbits the Sun in the outer asteroid belt at a distance of 2.7–3.5 AU once every 5 years and 4 months (1,961 days; semi-major axis of 3.07 AU).