The galaxy presents as a diffuse, moderately bright object with a disturbed morphology. It has an irregular shape, lacking a well-defined structure such as spiral arms or a prominent bulge. The central region appears somewhat smooth and more concentrated, while the outer regions exhibit a clumpy texture with what appear to be multiple knots or irregular features. There are hints of blue light, particularly in these outer regions, indicative of recent or ongoing star formation. The galaxy may be undergoing a minor or major merger based on the disturbed morphology.
