The galaxy presents as a spiral structure, though somewhat disrupted. A distinct central bulge is observed, appearing bright and concentrated. The spiral arms are not fully defined; some segments show evidence of disruption, potentially due to gravitational interactions or internal processes.

The galaxy exhibits a noticeable blue hue, suggesting the presence of relatively young, hot stars. A dust lane is suspected, though not well-defined. Patches of varying brightness are apparent across the disk, potentially indicative of HII regions or star-forming areas. Some distortion or asymmetry is present in the overall galactic shape.
