This galaxy appears to be a disk galaxy, observed at a high inclination, close to edge-on from our perspective. The central bulge is subtly visible, gradually transitioning into the surrounding disk. The galaxy exhibits a smooth, relatively featureless structure with a faint blueish hue, possibly indicative of ongoing, though subdued, star formation activity. There are no prominent dust lanes or spiral arm structures apparent, suggesting a more evolved system with a lower gas content. The morphology suggests it is unlikely undergoing any significant merger activity or major disturbances.
