The galaxy presents as a complex system, possibly undergoing a minor merger or interaction. There is a larger, somewhat amorphous central component that appears yellowish in color, which may indicate an older stellar population. Adjacent to it is a smaller, more elongated structure with a bluish hue. This bluer color suggests the presence of younger, hotter stars, perhaps fueled by a recent burst of star formation triggered by the interaction. 

The larger component exhibits a relatively smooth, featureless appearance. It lacks distinct spiral arms or a prominent bar structure. The general morphology hints at a possible transition state, evolving perhaps from a spiral towards a more elliptical form. The overall structure is not perfectly symmetrical, which could be another indication of gravitational disturbance from a nearby companion.
