The galaxy presents as a spiral type, with a central bulge that appears relatively small to moderate in size. The arms are fairly prominent, exhibiting a loosely wound structure extending outwards from the central region. There is an indication of two main spiral arms. The galaxy is viewed at an angle, as it is not fully face-on or edge-on. No major distortions or signs of a significant merger event are readily apparent, although subtle disturbances cannot be ruled out. A faint bar structure may be present across the central bulge. The spiral arms appear to have numerous active star-forming regions, judging by the blue hue present within them. 
