The galaxy appears to be an interacting system, possibly in the early stages of a merger. Two distinct luminosity concentrations are observed, suggesting two separate galactic nuclei. One nucleus displays a bluer color, indicative of a younger stellar population and possibly ongoing star formation, while the other exhibits a more yellow/red hue which is typical of older stellar populations. There is a stream of faint light connecting the two galactic centers, likely composed of stars and gas pulled between the two interacting galaxies via tidal forces. The overall morphology is disturbed and irregular, deviating significantly from a typical elliptical or spiral form. The system exhibits a relatively smooth light distribution around the nuclei and connecting tidal feature with minimal distinct features or spiral arms present.
