The galaxy presents as a well-defined spiral galaxy with a noticeable disk structure. It is inclined relative to our line of sight. The central bulge is prominent and appears yellowish-white, suggesting an older stellar population. The spiral arms are tightly wound and well-defined, with some branching apparent. There is evidence of recent star formation within the spiral arms, indicated by blueish regions. The overall morphology suggests that the galaxy has not undergone any recent major mergers, although some minor tidal disturbances may be present.
