The galaxy presents a prominent disk-like structure, inclined significantly to our line of sight. Spiral arms are readily apparent, exhibiting a degree of symmetry. The winding of these arms appears to be moderate, not tightly wound nor extremely open. A central bulge is present, but it does not dominate the overall structure, appearing relatively small in proportion to the disk. There is no strong bar feature visible extending from the central region, although a subtle, less defined linear structure may be present. The disk exhibits clumpy regions, suggesting active star formation. A slight asymmetry in the overall morphology may indicate a possible past interaction or minor disturbance. The absence of obvious tidal tails suggests that if a merger or interaction occurred, it was either minor or in the distant past.
