The galaxy appears to be in a transitional state, possibly undergoing a significant interaction or merger event. The system presents with an irregular morphology, displaying a mixture of smooth and less defined structures. A dominant, relatively smooth component is visible, exhibiting a yellowish hue, suggestive of an older stellar population. Adjacent to this primary component, there appears to be a more diffuse, fainter region with a hint of bluer color, potentially indicative of ongoing star formation. The overall shape deviates significantly from a typical spiral or elliptical galaxy, leaning more toward a disturbed or merging classification. The light distribution is not uniform, showing clumpy concentrations of luminosity. Some tidal features are also apparent, indicating the existence of disruptive forces that are influencing the structure. Although no obvious spiral arm structures are observed, there is an indication of some disorganization within the system, lending credence to the interaction or merging scenario.
