The galaxy presents a complex morphology indicative of an ongoing or recent merger event. Two distinct, bright, yellowish galactic nuclei are observed, suggesting the presence of two progenitor galaxies. The overall shape appears disturbed, lacking a clear spiral or elliptical structure, as it displays an irregular form. Faint tidal tails or streams of stellar material extend outwards from the main body, indicating gravitational interactions. The color indices suggest a mixture of stellar populations, with older, redder stars concentrated in the nuclei, and bluer, younger stars potentially associated with regions of active star formation in the disrupted disk and tidal features. There's also a faint, wispy arc of material encompassing part of the interacting galaxies.
