The galaxy appears to be undergoing a significant disturbance, possibly due to a merger event. The core region exhibits a concentrated, yellowish-orange hue, suggesting a population of older stars. From the core, a fainter, elongated structure extends outward. This extended structure shows a bluish tint indicating regions of potential active star formation. There is a noticeable asymmetry in the outer structure. Patches of irregular intensity suggest a non-uniform distribution of matter within the galaxy. Overall, the galaxy does not appear to be a well-defined spiral or elliptical.
