The galaxy presents a largely smooth morphology, appearing approximately round in shape. There is a hint of a disk-like structure. Based on color gradients, the central regions seem to have a redder hue, possibly indicating an older stellar population. The outer regions appear slightly bluer, which could indicate areas of more recent star formation. There is no prominent spiral arm structure visible. There is no evidence of a major merger event, though there is a hint of a minor disturbance to the galaxy shape.
