The galaxy presents as a disturbed system, with a morphology suggesting an ongoing or recent merger event. There are two distinct, irregularly shaped luminous components that appear to be interacting. Each component displays a diffuse, bluish hue, suggestive of relatively recent star formation. A tidal tail or bridge of material is seen extending outwards from one of the components, indicating gravitational disruption. The overall structure lacks a well-defined nucleus or spiral arm structure, which is consistent with the merger hypothesis. Given the irregular morphology and blue coloration, the galaxy is likely undergoing a period of enhanced star formation triggered by the interaction.
