The galaxy exhibits a morphology that suggests it is undergoing or has undergone a significant interaction or merger. The core region is dominated by a bright, relatively smooth concentration of light, appearing slightly elongated. This central structure is surrounded by more diffuse, irregular features. There is evidence of a tidal tail or disrupted arm extending from the main body, indicating gravitational disturbance. Patches of bluer light are scattered throughout the galaxy, suggestive of ongoing star formation regions, especially prominent in the distorted features. The overall color index suggests a mixture of stellar populations, with both older, redder stars and younger, bluer stars present. The lack of a well-defined spiral structure indicates that this is likely not a grand-design spiral galaxy. The galaxy appears relatively compact, though the faint extensions suggest a wider spatial extent than immediately apparent. The galaxy exhibits a morphology with both smooth and disrupted features, as well as both young and old stellar populations.
