The galaxy exhibits a distinct disk-like structure, though its orientation is not perfectly edge-on, revealing features within the plane. Spiral arms are clearly present, appearing somewhat tightly wound. A central bulge is visible, it appears to be of moderate size. The galaxy presents an overall blue hue, suggesting active star formation. There are indications of tidal interactions, with a significant amount of light being contributed from what appears to be a second object and disrupted morphology. There is evidence of a possible bar structure crossing the central region of the galaxy. The system shows no strong signs of violent merging but appears to be disturbed.
