The galaxy exhibits a generally amorphous morphology. Its overall color is a mix of blue and green hues concentrated in the center, suggesting the presence of a younger stellar population and potential ongoing star formation within a radius of approximately 3 kpc. Distortions are present in the outer regions, indicating a potential past or ongoing interaction, possibly a minor merger event. One area appears to have a more reddish color, which hints at an older stellar population or dust obscuration. The structure is not clearly disk-like, but appears to be a more irregular shape, perhaps a result of the recent merger. There are disturbances and signs of ongoing dynamic processes within the system.
