The galaxy presents as a spiral galaxy with a clearly defined, bright central bulge. The bulge appears relatively smooth. Faint spiral arms extend outwards from the central bulge, showing moderate winding. These arms appear somewhat flocculent, with hints of blue knots, suggesting regions of active star formation. The disk appears to be viewed nearly face-on. There are some signs of a possible weak bar structure extending across the galaxy's center. Overall, the galaxy displays a morphology indicative of a late-type spiral.
