The galaxy appears to be a spiral galaxy, viewed at a significant angle. The central bulge is prominent and exhibits a yellow-white hue, suggesting an older stellar population.  Spiral arms are faintly visible, displaying a mottled blue color, indicative of ongoing star formation.  The overall structure is somewhat disturbed or irregular.  There is evidence of tidal features or possible interactions, with a slight asymmetry in the galactic disk. Dust lanes are subtly visible within the spiral arms, obscuring some of the background starlight. Star formation seems moderately high. The galaxy appears to be undergoing some sort of merger event, with the general shape distorted, and possibly two distinct bulges.
