This galaxy exhibits a disk-like morphology with prominent features indicative of ongoing interaction or disturbance. A central, relatively smooth and bright region suggests a galactic bulge, though it appears elongated rather than spheroidal. The disk structure shows a distinct blueness, possibly representing active star formation regions containing populations of young, hot stars. 

Arms are not clearly defined, but there are asymmetrical extensions of light emanating from the main body of the galaxy. One appears as a tail or plume, potentially a tidal feature resulting from a past or ongoing gravitational interaction. The overall structure is irregular, lacking the grand design spiral structure commonly observed in isolated disk galaxies. The light distribution across the galaxy suggests significant asymmetry and potential morphological disruption. It may be involved in a merger event or a close encounter with another galaxy, given the disturbed morphology.
