This galaxy presents a primarily disk-like structure with a relatively small bulge. The spiral arms are tightly wound and well-defined, exhibiting a two-armed morphology. Patches of active star formation are evident within the arms, appearing as brighter regions. The galactic disk is the dominant feature, showing a slight inclination relative to our line of sight. It appears the galaxy is not undergoing any major merging events, although some minor disturbances may be present. A weak bar structure is observed in the galaxy's center.
