The galaxy appears as a relatively bright, disk-shaped object. The central region exhibits a strong concentration of light, indicative of a prominent galactic bulge or active galactic nucleus. The disk component surrounding the core appears relatively smooth, with some hints of spiral arm structures. The galaxy's color profile suggests a mix of stellar populations, with a dominant blue-green hue suggesting recent or ongoing star formation, and a slight hint of older, redder stars within the central bulge. There may be a slight disturbance to the galaxy, as evidenced by minor asymmetries. Overall, the galaxy is likely a spiral galaxy, with some peculiarities to its structure.
