The galaxy presents as a well-defined spiral, exhibiting a clear disk structure with a prominent bulge. The spiral arms are tightly wound, displaying a flocculent morphology with patchy regions of star formation. There are a large number of arms that are difficult to completely resolve. The bulge appears relatively small in relation to the overall disk size. The galaxy is tilted at an angle, providing a near face-on view. Dust lanes are visible within the spiral arms, contributing to the patchy appearance. Overall color indices suggest a mix of stellar populations, with a central concentration of older, redder stars and bluer regions indicating ongoing star formation in the spiral arms. No signs of major mergers or significant tidal distortions are apparent.
