The galaxy presents a spiral morphology, viewed at a slight inclination.  Well-defined spiral arms emanate from a relatively small, central bulge. These arms appear grand design, although some disruption is seen. The galaxy has some flocculence. The central bulge exhibits a yellowish hue, suggestive of an older stellar population. Spiral arms exhibit a bluish tint with some areas of greater redness, indicative of ongoing star formation and the presence of younger, hotter stars. The disk is bright with hints of dust lanes. The arms are tightly wound and extend considerably from the central region, indicating a relatively evolved state. The galaxy does not appear to be strongly barred but there may be a weak bar. There's no clear visual evidence of a major interaction or merger event in this image, but the arms may indicate some minor past disturbance. The galaxy presents a moderate concentration, with a small bulge.
