This galaxy exhibits a spiral morphology. The arms appear well-defined and emanate from a central region. The winding of the spiral arms appears to be moderate, not tightly wound nor loosely dispersed. A hint of a bar-like structure may be present in the central region of the galaxy, spanning a moderate length. A bulge component is observed, although it does not dominate the galaxy's overall structure. The galaxy does not appear to be undergoing a major merger, but there appears to be slight asymmetry or disturbance in the outer regions of the disk, indicating a possibility of a minor disturbance due to tidal interactions with smaller galaxies. Star forming regions are present throughout the arms, specifically in red and blue hues. The galaxy itself is an average size, and the color shows active star formation. 
