The galaxy appears to be a spiral galaxy, viewed at a near edge-on inclination. A prominent central bulge dominates the morphology, exhibiting a smooth, concentrated light profile. The disk component is faint and tightly wound, possibly due to the edge-on view. The dust lanes are subtle. Some features might indicate minor disturbances, possibly a small ongoing merger or tidal interactions. The galaxy exhibits a smooth, red color, suggesting an older stellar population and low star formation.
