The galaxy presents as a flocculent spiral, exhibiting fragmented and discontinuous spiral arm segments. A discernible, though not overwhelmingly dominant, central bulge is apparent. The arms are populated with numerous regions of intense blue light, likely indicating active star formation occurring within. The overall color of the galaxy suggests a relatively recent episode of star formation. The disk appears to be viewed at a somewhat inclined angle. There are potentially indications of a minor merger event or tidal disturbance present, although the evidence is not conclusive from this image alone. There is a notable presence of neutral hydrogen gas in the galaxy.
