This galaxy exhibits a distinct spiral structure with a noticeable central bulge. The spiral arms appear somewhat tightly wound, showing active star formation, indicated by the presence of bluish regions within the arms. These regions likely contain populations of hot, young stars. The galaxy is observed at a slight inclination, providing a partial view of its disk. The central bulge exhibits a yellowish hue, suggesting an older stellar population. The galaxy displays a moderate level of internal activity, with a substantial disk component contributing to its overall luminosity. There is no obvious presence of bars in this image. The morphology suggests a relatively undisturbed system, without signs of major interactions or mergers, although minor disturbances cannot be ruled out.