The galaxy presents as a roughly elliptical structure with a bright, concentrated central region. This central area exhibits a bluish-white hue, suggesting a potentially high concentration of young, hot stars or active galactic nucleus activity. 

Extending outward from the central region is a fainter disk-like component. This disk shows some mottled structure, possibly indicative of dust lanes or regions of varying stellar density.

Overall, the galaxy's color appears somewhat blueish, though not strongly so. This would indicate moderate amounts of young stars or a relatively low amount of dust obscuring the galaxy. There is a suggestion of some disturbance present in the structure of the disk.
