The galaxy presents as a face-on spiral, though the spiral structure is not sharply defined. A central bulge is prominent, displaying a yellowish hue, suggesting an older stellar population. Surrounding the bulge, the disk appears somewhat flocculent, with indistinct spiral arms and varying concentrations of blue light. Patches of what could be star-forming regions, exhibiting a bluish tint, are sparsely distributed throughout the disk. The overall morphology indicates a possible intermediate stage of evolution, displaying characteristics between a well-defined spiral and a more irregular form. There is a weak suggestion of a bar-like structure. Based on the disturbed morphology there may be a possible minor merger event or internal disturbance.
