This galaxy appears to be undergoing a significant interaction or merger. It exhibits a disturbed morphology, presenting as two primary luminous components that are closely associated. The overall shape is irregular and deviates significantly from a typical disk or elliptical structure. The galaxy appears relatively smooth, and the luminous components are likely concentrations of older stellar populations. There are indications of tidal features extending from the central components, suggesting gravitational disruption due to the interaction. Star formation appears to be relatively low, evidenced by the lack of strong blue emission associated with young stars. The overall color is redder, consistent with an older stellar population.
