The galaxy presents as a somewhat asymmetrical spiral. A central bulge exhibits a yellowish-white color. The spiral arms are not sharply defined, appearing more as diffuse, bluish regions extending from the central bulge. There is evidence of active star formation within these arms, indicated by the blue hue. The overall structure suggests a relatively mature galaxy with ongoing, moderate star formation. There may be some minor gravitational disturbance, as the disk does not appear perfectly regular. 
