The galaxy presents as a spiral, exhibiting a noticeable disk structure. The disk itself shows a slight inclination relative to our line of sight, offering a partial view of the spiral arms. These arms appear tightly wound and traced with regions of active star formation, indicated by their bluer color. A central bulge is present, exhibiting a yellow/orange hue, suggesting an older stellar population and less ongoing star formation activity compared to the disk. Overall, the galaxy displays a moderate level of internal structure and a moderately sized bulge.
