The galaxy appears to be an interacting system, possibly in the late stages of a merger. There is a relatively smooth, elliptical component showing a yellow-orange hue, suggesting an older stellar population with little current star formation. This component appears roughly spherical.

The second component presents a bluer color, with a more elongated, disk-like morphology. While it's difficult to discern detailed structure, it is possible this component is a spiral galaxy. The overall shape is suggestive of tidal interactions disrupting the disk structure.

The tidal interactions are likely triggering bursts of star formation within the bluer component. The galaxy system is relatively compact, indicating a close interaction. There is a hint of a tidal tail or bridge connecting the two components, or perhaps a shared halo. The spatial extent of the system is relatively small.
