The galaxy presents as a spiral galaxy with well-defined spiral arms. The arms are tightly wound and appear to originate from a bright, moderately sized central bulge. The galaxy displays a distinct disk structure. The disk does not appear to be edge-on. The spiral arms exhibit a generally organized structure, primarily featuring two dominant arms. Some distortions and faint, diffuse features are apparent within the disk, potentially indicating minor interactions or disturbances. No strong bar structure is evident within the central region. The arms show some hint of star formation.
