The galaxy presents as a moderately bright, disk-shaped structure. The central region is a relatively featureless bulge. The majority of the galaxy is a yellow white hue, with low surface brightness. The disk shows hints of spiral structure, although the arms are not well-defined. The overall impression is that of a spiral galaxy undergoing a period of relative quiescence, or one which is dominated by older stellar populations. It is elongated and oval in shape. There is no obvious evidence of a recent major merger, although some minor disturbances in the disk cannot be ruled out based on this image alone.
