The galaxy appears as a smooth, elongated structure with a cigar-shaped morphology. Its light profile suggests a central bulge that gradually fades into the surrounding galactic disk. The color distribution indicates a concentration of older stellar populations toward the center, evidenced by a yellowish-orange hue, while the outer regions exhibit bluer tones, possibly indicating more recent star formation. No distinct spiral arms or bar structures are discernible. There is a hint of disturbance on one side.
