The observed galaxy exhibits a notable smoothness in its overall morphology, suggesting a relatively evolved system. There appears to be a binary system composed of two objects, most likely the galactic nucleus and a large area of star formation, and that appear roughly spherical. The system is dominated by redder wavelengths, implying a population of older stars. The observed system appears to be undergoing some kind of merging, as there is a connection of material between the two observed spherical components. The overall shape tends to have a round appearance. It exhibits a relatively low star formation rate. The combined mass of both spherical objects is estimated to be substantial.
