The galaxy displays a complex morphology indicative of an ongoing or recent interaction. The primary body of the galaxy exhibits a central, bright core, possibly a galactic bulge. A disk-like structure appears present, however it is distorted and irregular. A prominent tidal tail arcs away from the main body, suggesting gravitational disruption. The tail appears diffuse and its color suggests a mixture of stellar populations, potentially triggered by the interaction. The galaxy shows a slight blueish hue, particularly in areas away from the core, which could indicate regions of recent star formation. There is indication of a minor merging event.
