The galaxy appears to be an edge-on spiral or lenticular galaxy. It presents a bright, concentrated central bulge that seems relatively smooth in texture and has a yellowish color, likely indicative of an older stellar population. Extending outward from the bulge is a fainter, elongated disk. The disk displays a bluer hue, suggesting the presence of younger, hotter stars. The disk region seems slightly disturbed, and exhibits asymmetric features. There's a faint hint of dust lanes or patchy structures within the disk. The galaxy appears isolated, with no clear signs of major tidal interactions or ongoing mergers. The overall morphology suggests an evolved system that may have undergone some minor disturbances.
