The galaxy presents a disk-like morphology, though somewhat disturbed. Evidence of spiral arm structure is visible, emanating from a moderately sized central bulge. The disk appears more prominent than the bulge, with a relatively low bulge-to-disk ratio. The arms are not tightly wound, displaying a more open, grand design structure. The disk exhibits some clumpy regions, potentially indicative of active star formation. There appears to be a bar-like structure that is weak, but bisects the central bulge. The galaxy is also displaying signs of a possible minor merger or tidal interaction, with some asymmetric features.