This galaxy exhibits a clear spiral structure. The arms are loosely wound and rather patchy, suggesting ongoing star formation. There are two dominant spiral arms. A central bulge is observable, appearing moderately sized, contributing significantly to the overall luminosity of the galaxy. There's some evidence of a minor interaction or disturbance influencing the galaxy's morphology, visible as subtle asymmetries within the arm structure. The disk is viewed at a slight angle, but not perfectly edge-on. 
