This galaxy exhibits a clear spiral structure with a moderately sized central bulge. The spiral arms are loosely wound, suggesting a relatively late-type spiral galaxy classification. Two prominent spiral arms are visible, originating from the central bulge and extending outwards. The presence of active star formation is suggested by the bluish-white color observed within the arms. A subtle bar structure appears to be present within the central region. No major morphological disturbances indicative of recent major merger events are apparent. Overall, the galaxy presents a well-defined spiral structure with moderate disk prominence and ongoing star formation.
