The galaxy appears as an elongated, disk-shaped structure seen nearly edge-on. There's a noticeable bulge at the center of the galaxy, possibly with a boxy appearance and a concentration of older, yellowish stars. The disk itself exhibits a bluer tint and signs of star formation, but no spiral arm structure is visible. The color suggests that the galaxy is undergoing significant star formation with a stellar mass typical for galaxies of this type. There is no indication of a major merger, or of any significant disturbances in the galaxy's structure.
