The galaxy presents a moderately perturbed morphology. Its overall shape is somewhat amorphous, displaying an irregular structure with a noticeable disturbance. A central, brighter region is present, possibly indicative of a galactic bulge or active galactic nucleus. The surrounding areas show a clumpy texture. The color distribution suggests some ongoing star formation, potentially concentrated in the bluer patches that are observed. There appears to be an active interaction or recent merger event affecting the overall structure of the galaxy. It does not present as a well-defined spiral or elliptical galaxy.
