The galaxy presents as a relatively face-on spiral. Two prominent spiral arms emanate from a central bulge, though the structure is somewhat disturbed or flocculent. The arms are moderately wound, displaying neither an extremely tight nor particularly loose morphology. The bulge appears moderate in size relative to the overall disk. A bar structure may be present, but is not strikingly pronounced. The disk displays a blue hue, suggestive of ongoing star formation. There appears to be little to no dust lanes visible. The overall luminosity suggests a galaxy of moderate mass and star formation activity. There is no clear evidence of a major merger, though minor disturbances cannot be ruled out based on the image alone.
