The galaxy presents an apparent disk-like morphology. The galaxy is faint, possessing a low surface brightness. There is a distinct absence of defined spiral arm structures, which gives it an irregular shape. The central bulge appears small relative to the overall disk. Color gradients are subtle, showing a slight variance in blue and green hues, possibly indicating differential star formation or dust distribution across the galaxy. There seems to be slight disturbance within the disk structure indicating a potential interaction or merger.
