The galaxy appears to be a spiral galaxy, viewed approximately face-on. The central bulge is a yellowish color, potentially indicating an older stellar population. Two prominent spiral arms are visible emanating from the central bulge, and their winding seems relatively tight. Some clumpy regions within the arms suggest areas of active star formation. The disk component is noticeably brighter than the immediate surroundings. The image suggests that the galaxy is not undergoing any major mergers, but some minor disturbances cannot be ruled out. The size of the bulge appears small compared to the disk.
