The galaxy appears to be in a late stage merger, possibly between two or more galaxies. There are two distinct, bright regions that likely represent the merging galactic nuclei. One nucleus is significantly more prominent and displays a bluer color, suggesting ongoing star formation. The other nucleus has a distinctly redder hue. The overall form is somewhat amorphous, lacking clear spiral structure, indicating a significant disruption of the galaxy's original morphology. A faint, extended tidal tail feature is noticeable connecting the two regions, further supporting the merger hypothesis. There may be faint hints of disturbed disk structure throughout the galaxy, but these are obscured by the merger event. The galaxy's morphology points towards a system where tidal forces are actively shaping its evolution.
