The galaxy exhibits a spiral morphology. Two arms are clearly visible, winding moderately tightly around a central bulge. The bulge appears small relative to the disk, and appears to have a pale yellow coloration. The arms are broad and somewhat diffuse, with a predominantly blue hue. The arms do not appear flocculent, but are largely a smooth structure with little sign of star forming regions, however the color of the spiral arms suggests they are home to numerous young, hot stars. There is no obvious evidence of a bar structure. No significant tidal distortions or merger features are apparent in the image, though one cannot exclude there having been a past interaction.
