The galaxy presents as a spiral type, with a discernible disk structure viewed at a slight angle, but not quite edge-on. The spiral arms are prominent, showing a tightly wound morphology. There appears to be ongoing star formation within the arms as evidenced by the regions of enhanced blue luminosity, indicative of younger, hotter stars. The central bulge is relatively small, and not a dominant feature of the galaxy's overall structure. No strong bar structure is readily apparent. There is no obvious morphological evidence of any major merging activity, although subtle disturbances may be present. The galaxy exhibits a generally smooth appearance, but featured due to the distinct spiral arm structure.
