The galaxy presents a somewhat irregular morphology, with a disk-like structure exhibiting notable disturbances. There is a suggestion of an edge-on orientation of the disk. A central bulge appears diffuse and elongated. The disk appears clumpy with luminous regions interspersed with areas of lower surface brightness. Overall, the galaxy shows a disturbed morphology suggestive of possible ongoing or recent interaction or merger events. Some bright regions may indicate zones of active star formation. Based on the apparent magnitude in various filters, we can infer it is a relatively large galaxy.