The galaxy presents with an irregular morphology, characterized by a disturbed structure. There is a central, brighter core exhibiting a yellowish hue. Emanating from this core is an extended, diffuse blueish emission, which appears somewhat elongated. Adjacent to the core, there is a fainter, more diffuse emission, possibly indicating a tidal tail or a smaller interacting galaxy. The overall structure suggests ongoing or recent merger activity, with signs of gravitational disturbance visible.
