The galaxy presents as a spiral type, viewed at a considerable angle away from face-on. There is a central bulge that appears relatively small. Spiral arms are clearly visible and appear tightly wound. The galaxy exhibits a distinct blue hue throughout the disk, indicative of ongoing star formation. A bar structure is not obviously present. There appear to be no signs of major mergers or significant tidal disturbances within the visible structure. Some areas of the arms are difficult to discern, perhaps due to dust obscuration or lower surface brightness.
