The galaxy displays a clear spiral structure. Two prominent spiral arms emanate from a central, bright bulge. These arms appear somewhat tightly wound around the bulge. The color gradients within the arms suggest varying stellar populations; bluer regions may indicate areas of more recent star formation, while yellower regions may host older stellar populations. The central bulge appears yellow-orange. The galaxy appears to be undergoing some form of gravitational disturbance, given the asymmetry and presence of extended tidal features or distorted spiral arms. There appears to be a bar feature across the galactic center. The galaxy is not seen edge-on but rather at an angle closer to face-on.
