The galaxy presents as a relatively compact spiral with a prominent central bulge region. The bulge appears moderately sized. There are indications of spiral arm structure extending outwards from the central bulge, exhibiting a somewhat disrupted morphology. Bright knots are visible within the arms, possibly indicating areas of active star formation. There are indications of tidal disturbances or interactions, which suggest that the galaxy may be involved in a merging event or that it has undergone a major disturbance. The disk is oriented at an oblique angle, which makes it difficult to discern its overall shape. There does not appear to be a strong central bar, though subtle bar-like features cannot be ruled out. Overall, the galaxy appears to be an actively evolving system, possibly undergoing interactions with another galaxy.
