The galaxy presents a distinct spiral morphology.  Spiral arms are clearly visible, emanating from a central bulge. The arms appear tightly wound around the galactic center, which suggests a classification as a late-type spiral galaxy.  The bulge is relatively small in comparison to the disk.  The disk is viewed at a slight angle, but not quite edge-on.  There is no sign of a significant bar structure.  The galaxy does not appear to be undergoing any major mergers or significant tidal disturbances, though there is very possibly a minor disturbance. Color gradients within the spiral arms are indicative of ongoing star formation. The outer regions exhibit a bluer hue, suggesting the presence of younger, hotter stars. The spiral arms themselves seem to be somewhat flocculent.
