This galaxy presents as a barred spiral type, viewed at an oblique angle. The disk is clearly visible, exhibiting prominent spiral arms with a noticeable degree of patchiness. The arms appear loosely wound, indicating possible flocculent structure. A central bulge is not very discernable, appearing small if present.

There's evidence of an interaction or merger event. The galaxy shows disturbed morphology. The light distribution is complex, with at least one tidal tail or bridge extending outward. There are also clumpy regions throughout the disk, which may be signs of recent star formation triggered by the interaction. Color gradients suggest a higher concentration of younger, bluer stars within the spiral arms. The overall color appears moderately blue, indicative of ongoing star formation. Dust lanes are not easily distinguished, although some obscuration may be present within the arms and near the central region.
