The galaxy presents a morphology characteristic of a spiral galaxy, exhibiting a distinct disk structure. Spiral arms are clearly visible, with a tightly wound appearance in certain sectors and a more open structure in others. Evidence suggests the presence of two dominant spiral arms. The central bulge is of moderate size relative to the overall galaxy, and it is uncertain whether a stellar bar is present, though the structure hints at one, indicating a possible weak bar. The disk appears to be observed at a significant inclination, but it is not close to edge-on. No signs of major mergers are apparent, though minor disturbances cannot be ruled out. Star formation appears active within the spiral arms, as indicated by the blue hue. Overall, the galaxy appears to be a relatively normal spiral galaxy, actively forming stars.
