The galaxy presents as a face-on spiral, exhibiting a distinct blue tint suggestive of active star formation regions within its spiral arms. A noticeable central bulge, exhibiting a yellow/orange hue indicative of an older stellar population, is present. While distinct spiral arm features are visible, they are not particularly tightly wound, displaying a rather grand design. There is no obvious indication of a strong bar structure bisecting the central bulge, though a weaker, less defined structure cannot be ruled out. Overall, the galaxy seems to be a fairly typical spiral galaxy in terms of morphology. Evidence of minor gravitational disturbances is visible upon close inspection of the spiral arm structure.
