This galaxy appears to be a spiral galaxy, viewed at a significant inclination. The central bulge is a bright, yellowish-white, suggesting an older stellar population. A faint, flattened disk extends outwards from the bulge, displaying a bluer hue indicating the presence of younger stars and possibly some ongoing star formation. The galaxy's overall structure is relatively smooth and undisturbed; with no obvious signs of major tidal interactions or ongoing mergers, though minor disturbances cannot be ruled out. The colors throughout the galaxy shift from yellows and reds in the center towards greens and blues as you move towards the edges. There is possibly a small amount of dust present in the disc. The galaxy's shape could suggest it is an earlier type spiral, with a dominant bulge.
