The galaxy presents as a spiral type, exhibiting distinct spiral arm structures. The arms are well-defined, displaying a predominantly two-arm morphology. A bar structure appears to be present, though not prominently, potentially of a weaker nature. The winding of the spiral arms is observed to be primarily of medium tightness.

The central bulge is notable, though not overwhelmingly dominant, exhibiting a moderate size relative to the disk. Evidence suggests active star formation within the galaxy, particularly in the spiral arms, as indicated by the presence of blue regions associated with young, hot stars.

There appears to be an interaction occurring, possibly a minor disturbance, based on the galaxy's shape.
