The galaxy exhibits a clear spiral structure. Two prominent spiral arms are visible, extending outwards from a bright, moderately sized central bulge. The arms appear to be wound relatively tightly around the bulge. A bar structure is visible, moderately strong in appearance, which spans across the center of the galaxy. The color profile indicates a likely older stellar population, particularly within the bulge and inner disk, showing a yellow-orange hue. The outer spiral arms display a more diffuse, slightly bluer coloration, suggestive of ongoing or recent star formation. There is no obvious signs of major disturbances or ongoing mergers, such as tidal tails or asymmetrical features, though some minor distortions within the disk cannot be fully discounted. Overall, the galaxy appears as a well-formed spiral galaxy with a moderate bulge and prominent spiral arms.
