This galaxy presents as a spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population. Spiral arms are clearly visible, displaying a bluish tint indicative of ongoing star formation. The arms appear tightly wound, and the system is close to face on, allowing for a good view of the spiral structure. There may be some disturbances visible, which could be from a potential minor merger. Overall, the galaxy presents a moderately inclined disk with an evident spiral structure dominated by a central bulge and active star formation.
