The galaxy presents as an edge-on spiral system, exhibiting a clearly defined disk. A prominent central bulge dominates the galaxy's core, appearing smooth and elongated. There is evidence of a slight warping in the galactic disk, indicative of potential gravitational interactions or internal dynamics. The disk appears relatively uniform in color, suggesting a more mature stellar population with lower rates of on-going star formation. A slight asymmetry is observed in the overall structure, which could be attributed to a minor gravitational disturbance or a past merger event. Based on the red color, we can estimate a moderate to high stellar mass.
