The galaxy presents a clear spiral morphology, with tightly wound arms emanating from a prominent central bulge. The spiral structure is well-defined, with multiple arms discernible. A bar-like structure bisects the central bulge. Dust lanes are observed along the inner edges of the spiral arms, contributing to the galaxy's overall contrast. The galaxy exhibits a blue hue, indicative of ongoing star formation within the spiral arms. The bulge region displays a yellowish color, suggesting an older stellar population compared to the arms. There are some minor disturbances/unevenness present in the spiral arms, possibly due to gravitational interactions or recent merging activity. The galaxy appears moderately inclined.
