The galaxy exhibits a complex morphology with a hint of a spiral arm structure, though significantly disrupted. The overall color gradient suggests ongoing star formation, particularly along the brighter sections of the possible spiral arms. The central region is less defined, appearing somewhat diffuse and redder in hue. Evidences of a minor interaction or recent merger events are visible. Patches of bluer light, indicative of intense star-forming regions, are scattered, suggesting a heterogeneous distribution of stellar populations. There is a strong indication of tidal disruption or the aftermath of a gravitational interaction. The galaxy's outer regions appear irregular and distorted, deviating from a classic spiral shape.
