The galaxy presents as a system undergoing a significant interaction or merger. Two distinct, luminous components are observed, each exhibiting a roughly elliptical morphology. The colour profile of the two components suggest older stellar populations are at play. There is evidence of potential tidal features or distorted morphology in each of the two components, indicating gravitational disturbances due to the ongoing merger process. The relative proximity and apparent distortion of the two nuclei suggests a strong gravitational influence between them. Based on the lack of strong blue colouration, a relatively low star formation rate is expected.
