The galaxy presents as a disk-like structure with evidence of significant disturbance and possible tidal interactions. The overall morphology is irregular, lacking the clear spiral arm structure of a grand design spiral. There is an apparent asymmetry in the disk, with one side appearing more extended or disrupted than the other. Within the main body of the galaxy, I observe regions of diffuse light, possibly indicative of ongoing star formation. The core region is not clearly defined, with no distinct bulge visible. I observe a faint, extended halo surrounding the main body, suggesting possible tidal debris or interaction with a nearby system. Overall, the galaxy appears to be in a state of interaction or recent merger activity, as evidenced by the disturbed morphology and lack of defined spiral structure.
