This galaxy appears to be a spiral galaxy seen at an oblique angle. It exhibits a prominent central bulge that appears orange in color, suggesting an older stellar population. The disk is visible, showing some asymmetry. One side of the disk presents a bluish hue, potentially indicative of ongoing star formation. There are some disturbances on the other side, possibly from interaction with another galaxy or recent activity. Overall, the galaxy's morphology suggests a transitional state between a spiral and potentially an elliptical galaxy, possibly due to a past or ongoing merger event. The shape is moderately elongated, deviating from a perfect circle.
