This galaxy displays a disturbed morphology, likely undergoing a significant merger event. The primary body of the galaxy exhibits a prominent central bulge surrounded by a disk structure. The spiral arms are readily apparent, displaying a range of winding tightness from tight to loose. Some of the arms have a flocculent structure. There is a second, smaller galactic structure close to the primary, displaying a bluer color. The presence of the bluer, smaller, galactic structure suggests a potential for ongoing star formation within these regions. The galaxy's overall color suggests a mix of stellar populations, with older, redder stars concentrated towards the bulge and younger, bluer stars located in the spiral arms. The galaxy is not seen edge-on. There appears to be a faint tidal tail extending outwards on one side, which is indicative of gravitational interaction. The dust lanes appear patchy and irregular.
