The galaxy presents a distinct spiral structure. Two prominent spiral arms emanate from a central bulge. The winding of the spiral arms appears relatively tight. The bulge itself exhibits a moderate size relative to the overall galactic disk. The disk appears to be presented face-on, exhibiting no apparent inclination. There is also an indication of minor disturbances, hinting at a possible interaction or past merger event. The blue color suggests active star formation within the spiral arms. The red-yellow tones indicate the presence of older, redder stars. A weak bar feature also appears to be present within the central region.
