The galaxy presents as an elongated structure, likely a spiral galaxy viewed edge-on. A prominent central bulge is visible, exhibiting a yellow-orange hue indicative of an older stellar population. Dust lanes appear to be present, though indistinct, obscuring some of the light along the galactic plane. Faint blue tinges at the far upper and lower edges indicate at least some on going star formation. No clear signs of major disturbances or mergers are apparent, although some subtle asymmetry may be present, hinting at a potential minor interaction in the past.
