The galaxy in the image exhibits a complex morphology, suggesting an ongoing or recent interaction or merger. The galaxy appears to be composed of two distinct components. One component is a smoother, more spheroidal structure, exhibiting a yellowish hue. This suggests an older stellar population with less ongoing star formation. The second component is more amorphous and displays a bluish tint, indicative of younger, hotter stars and ongoing star formation.

There are signs of tidal features or disturbances, such as faint extensions or asymmetries in the galaxy's outer regions. The overall shape of the system is irregular, deviating significantly from a regular elliptical or spiral form. This further supports the hypothesis of a merger or interaction. The relatively high star formation rate, inferred from the blue color, coupled with the disturbed morphology, points towards a system actively evolving due to gravitational interactions.
