The galaxy presents a notable spiral structure. Distinct, well-defined spiral arms emanate from a central bulge. These arms show areas of intense star formation, indicated by the blue color. The morphology is that of a spiral galaxy with a noticeable, but not overly prominent, central bulge.

The galaxy is observed face-on, allowing for a clear view of its spiral structure. There is evidence of ongoing star formation within the spiral arms, suggested by their color and patchy appearance. The overall color suggests that the object is a barred spiral, but the bar is not particularly distinct. The nucleus appears relatively bright and concentrated. There may be a weak or faint central bar.

The galaxy does not show signs of major interaction or disturbance. The disk is relatively undisturbed.
