The galaxy presents a prominent spiral structure. The spiral arms are well-defined and extend outwards from a central bulge. The arms exhibit a clumpy morphology indicative of ongoing star formation. The bulge has a moderate size, with some yellow color, suggesting it contains an older stellar population. The galaxy is inclined relative to our line of sight, but it does not seem to be edge on. There is no apparent major disturbance or interaction with other galaxies, nor is it a pure smooth galaxy. A faint stellar bar could potentially be present in the core, although the presence of a bar is questionable from a visual inspection alone. 
