The galaxy presents a morphology suggesting it is undergoing, or has recently undergone, a significant interaction or merger. The central region exhibits a bright, relatively amorphous structure with a blue hue, indicative of potential ongoing star formation. Extended, albeit faint, features are visible, suggesting tidal tails or disrupted arms. These extensions are not symmetrical, lending credence to the merger hypothesis. The galaxy's overall shape is irregular, lacking a well-defined spiral or elliptical structure, which is consistent with a disturbed system. The overall color profile suggests the presence of both older stellar populations (more red) and younger, hotter stars (blue).
