The galaxy presents as a disk-shaped system viewed at an oblique angle. There is a central bulge region that appears relatively bright and concentrated. Surrounding the bulge, the disk exhibits a mottled texture, suggesting the presence of spiral arm structures, although they are not sharply defined. The galaxy displays a blueish hue overall, with slight variations in color across the disk, possibly indicative of varying stellar populations or dust lane distribution. The galaxy's light profile gradually fades from the central region towards the edges, indicating that the stellar density decreases radially outwards.
