This galaxy appears to be an interacting system or a galaxy undergoing a merger. The main body exhibits a largely smooth morphology, though with some features indicating disturbance. There is a slight elongation suggesting it is neither perfectly spherical nor a thin disk, but somewhere in between. One prominent feature is a second concentration of light within the galaxy, suggestive of a second core or merging component. Patches of bluer light are visible throughout the galaxy, hinting at regions of on-going star formation. The overall color indices suggest the presence of a significant population of older stars. It exhibits irregularities in its overall shape, and lacks defined spiral arms or a clear elliptical structure.
