This galaxy presents a complex morphology, suggestive of an ongoing or recent interaction. The central region exhibits a bright, concentrated luminosity, potentially indicative of a significant stellar population and possible active galactic nucleus, or just a bulge in the center. Distinct, extended spiral arm structures can be discerned, although they appear disrupted and distorted. One prominent arm extends outward, exhibiting a notable curvature. Fainter, diffuse structures are also visible, possibly tidal tails formed from gravitational interactions. The overall color profile suggests a mix of stellar populations, with bluer regions in the arms, potentially indicative of more recent star formation, and a redder core, suggestive of an older stellar population. There are also regions that appear to be overlapping and in front of each other within the galaxy.
