The object appears to be a spiral galaxy viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellow-orange hue, suggesting an older stellar population. Dust lanes, although not sharply defined, are apparent along the galactic plane, obscuring some of the light from the bulge. The disk is relatively thin and elongated, appearing smooth with low surface brightness at its outer edges. The galaxy does not appear to be undergoing a major merger or significant tidal disruption.
