The galaxy presents a complex and disturbed morphology. Its central region is dominated by a bright, somewhat diffuse, and blue-tinged area, suggestive of recent or ongoing star formation. There is also a strong suggestion of merger activity. One distinct and elongated structure is seen extending away from the center, possibly a tidal tail or a disrupted arm. This extension has a smoother appearance, and a different color balance which may suggest an older population of stars. 

The overall shape appears elongated, cigar-shaped, which supports the possibility of an ongoing or recent merger event. The system is not well-defined and lacks a clear spiral structure. A merging or interacting companion seems likely.
