The galaxy presents as a likely disk galaxy viewed nearly edge-on. A prominent central bulge is visible, appearing mostly smooth and somewhat rounded. The disk itself exhibits a relatively uniform color gradient, with a possible faint dust lane or obscuration visible along the plane of the disk. Hints of structural disturbance or faint tidal features may be present on one side of the galaxy, suggesting potential past interaction or merger event, although the smoothness in one side could also be due to higher star formation rates or differing dust levels. Overall, the galaxy appears moderately bright.
