The galaxy presents an edge-on disk morphology. A prominent bulge dominates the central region, exhibiting a yellowish hue. The disk itself appears elongated and relatively thin, extending outwards from the bulge. There is a strong suspicion of a minor merger occurring within the disk. Possible signs of disturbance are visible, although the overall structure maintains a degree of regularity. There is a noticeable presence of dust along the galactic plane.
