The observed galaxy appears to be undergoing a significant merger event. Two distinct nuclei are visible, both exhibiting a yellowish hue, suggesting a population of older stars. The overall shape is highly disturbed, lacking a clear spiral or elliptical structure. There are faint blueish wisps in between the two nuclei, which may indicate regions of active, but weak star formation. Based on the disturbed morphology, this system is likely in the late stages of merging. The galaxy is quite massive and shows to have very low ongoing star formation.
