The observed galaxy appears to be a spiral galaxy viewed edge-on. There is a prominent central bulge that appears relatively smooth and elongated, displaying a yellowish-orange hue, indicative of an older stellar population. The disk of the galaxy is highly inclined relative to our line of sight. The disk displays shades of blue, possibly indicating the presence of younger, bluer stars and active star formation. No distinct spiral arm structures can be identified due to the edge-on orientation, but the outer regions of the disk appear slightly irregular, possibly indicating minor disturbances or interactions. The overall morphology suggests a system with a significant disk component and moderate to high stellar mass.
