The galaxy presents as a spiral galaxy with a distinct structure. It is observed nearly face-on. The central bulge is prominent and exhibits a yellowish-white color, suggesting an older stellar population. The spiral arms are well-defined, appearing tightly wound and exhibiting a predominantly bluish hue, indicative of active star formation regions. Dust lanes appear to traverse the spiral arms, obscuring some of the starlight. The arms display a granular texture, characteristic of individual star clusters and HII regions. The galaxy lacks any obvious signs of a major ongoing merger event, although some minor disturbances cannot be ruled out. Overall, the galaxy appears as a well-formed spiral with ongoing, though possibly not extremely vigorous, star formation within its arms.
