The observed galaxy presents as a distinct, elongated structure oriented approximately vertically in the frame. Its morphology suggests it is a spiral galaxy viewed nearly edge-on. A central bulge is visible, exhibiting a yellowish-orange hue, indicative of an older stellar population. From the geometry and colors of the galaxy, the bulge appears rounded. The disk component is tightly wound and primarily blueish, suggesting the presence of on-going star formation within. The galaxy is fairly symmetric, with no apparent signs of major tidal disruption or recent merger events. Faint spiral arms can be barely discerned at the outermost parts of the disk, but they are highly flattened.
