The galaxy presents as a compact, relatively small object. It exhibits a noticeable blue hue, which may indicate ongoing star formation activity within. The morphology appears disturbed; the light distribution is not smooth, and there are suggestions of multiple nuclei or bright knots. The central region is brighter and somewhat elongated, potentially indicative of a disk-like structure viewed at an angle. Faint extensions or tidal features are possibly present, suggesting a recent or ongoing interaction or merger event. There may be faint arms or some other kind of disturbance that is hard to make out. Overall, the galaxy does not appear to be very large or perfectly elliptical.
