This galaxy exhibits characteristics suggesting an ongoing or recent merger event. Two distinct, luminous cores are visible, indicating the presence of two separate galactic nuclei in close proximity. The overall morphology is disturbed, lacking a clearly defined spiral or elliptical structure. Faint tidal features, possibly indicative of gravitational interactions, may be present in the outer regions of the galaxy. The color appears to be generally yellowish-red, which could imply a population of older stars and relatively low levels of on going star formation. The object exhibits a relatively high degree of smoothness with slight disturbance, and it is more rounded than not. Overall, the galaxy presents as a gravitationally interacting system with a high probability of merger activity.
