The galaxy presents as a face-on spiral with a discernible disk structure. A central bulge appears relatively small. The spiral arms are tightly wound, displaying a flocculent morphology with regions of active star formation, evidenced by the presence of blue knots along the arms. These regions suggest ongoing or recent bursts of star formation within the spiral arms. The overall color of the galaxy leans towards the blue end of the spectrum, indicative of a younger stellar population.
