This galaxy exhibits a clear spiral structure. The spiral arms are tightly wound and appear to extend outwards from a central bulge. The central bulge appears to have a moderate size relative to the disk, which has an approximately elliptical shape. The galaxy's disk component displays a range of colors, with regions of blue indicating potential areas of ongoing star formation. The overall morphology suggests a galaxy that is not currently undergoing any major mergers, although there may be some minor disturbances.
