The galaxy appears to be undergoing a merger, exhibiting signs of significant tidal disruption. Two distinct galactic nuclei are discernible, suggesting a recent or ongoing collision of two galaxies. One nucleus appears relatively compact and exhibits a yellowish-white hue, indicative of an older stellar population. The other nucleus is less defined and exhibits a bluer color, implying the presence of younger, hotter stars.

A faint stellar stream or tidal tail extends from the system, further supporting the hypothesis of a merger event. Overall, the morphology of the galaxy is highly irregular and perturbed, lacking a clear spiral or elliptical structure. There is evidence of enhanced star formation within the system, particularly in the vicinity of the bluer galactic nucleus.
