The galaxy presents as a spiral, observed at a moderate inclination. Two main spiral arms are clearly discernible, although their structure appears somewhat flocculent. Star formation appears to be present in the arms, with a strong suggestion of active star formation within the arms. The central bulge is relatively prominent, and appears to be composed of older stars. There's no obvious signs of active galactic nuclei activity, nor any obvious signs of major galaxy interaction or ongoing merging events, although I can see that there could be some minor disturbances within the disk. A very slight bar like feature appears present. The winding of the spiral arms appears to be somewhere between tight and loose.
