The galaxy presents as a spiral type, viewed at an angle, likely approaching face-on. Two spiral arms appear to emanate from a moderately sized central bulge. The bulge has a yellowish hue, suggestive of an older stellar population. The spiral arms are clearly defined and exhibit a loosely wound structure. The arms show clumpy regions of blue light, consistent with ongoing star formation. No significant dust lanes are observed. The galaxy appears relatively undisturbed. The image indicates it is not currently undergoing a major merger event. A bar structure may be present, but more detailed observations are required to confirm this.
