The galaxy appears as a single, relatively smooth object. There is a slight elongation, but overall it presents a rounded morphology. No distinct spiral arms or a prominent central bulge are readily discernible in the image. A subtle color gradient is present, with a slightly brighter and yellower core region. There is a faint blue tint to the outer regions of the galaxy, suggesting the presence of a small amount of on-going star formation. The overall structure indicates the galaxy could be in the early stages of a merger, or be a disturbed spiral galaxy.
