The galaxy exhibits a complex morphology, appearing as a likely merger event or a galaxy with significant tidal disturbances. The overall color profile suggests a significant population of older stars, with a reddish hue prominent in certain areas. Evidence of bluer, younger stars exists, particularly in regions that appear more disturbed or possibly areas of active star formation triggered by the interaction. There is an asymmetrical distribution of light, indicating it is not a simple elliptical or spiral. A tidal tail-like structure extending from the main body suggests a gravitational interaction, potentially with a nearby dwarf galaxy or another larger system. Patches of intense color variation may point towards areas of increased dust obscuration and varying star populations. The galaxy does not appear to have a well-defined nucleus.
