The galaxy appears to exhibit a disk-like morphology, though significant disturbances are present. There is likely a spiral arm structure, given the relatively even distribution of light around the center of the object. The arm structure appears significantly disrupted, with distortions and asymmetries visible. There is a slight concentration of light toward the core of the galaxy, which is difficult to fully discern. There is evidence of some ongoing or recent merger activity, as indicated by the asymmetry and potential tidal features. Overall the features are indicative of some level of recent interaction or gravitational disturbance affecting the system.
