The galaxy presents a moderately inclined, disk-like morphology. It appears to be a spiral galaxy, though its structure is not well-defined. There is evidence of a central bulge, slightly brighter and more concentrated than the surrounding disk. The disk itself displays some clumpy regions, possibly indicative of active star formation. The color of the galaxy appears slightly blueish, suggesting the presence of younger stellar populations. No pronounced spiral arms are observed. The overall appearance is that of a galaxy undergoing some degree of interaction or disturbance, but without any obvious major merger events. The surface brightness of the disk is relatively uniform, with some slight variations suggesting variations in stellar density or dust content.
