The galaxy presents a complex morphology, appearing as a spiral galaxy with indications of significant disturbances. A central bulge region is evident, displaying a smooth, concentrated light distribution. The spiral arms are not well-defined but appear flocculent and somewhat disrupted, suggesting ongoing interactions or internal processes affecting the galactic structure. The color distribution suggests a mixture of stellar populations, with bluer regions possibly indicative of recent star formation in the arms. A hint of possible tidal features or plumes extending from the main body is also present, further indicating a merger event.
