The galaxy displays a clear spiral structure, with two prominent spiral arms emanating from the central region. The spiral arms exhibit a somewhat flocculent morphology, with regions of active star formation visible as bluish knots. The spiral arms are moderately wound, showing a somewhat open structure.

The central bulge is relatively small compared to the overall size of the disk. There is a possible indication of a bar structure extending across the center of the galaxy, with a higher concentration of light oriented along the length of the bar.

There is no obvious sign of recent major merger activity or significant tidal disturbances. The overall color suggests a mix of stellar populations, with ongoing star formation as well as older, redder stars. Patches of dust are visible as dark lanes within the spiral arms, further obscuring the light from the stars.
