The galaxy appears to be a lenticular or early-type spiral galaxy, viewed at an oblique angle. The galaxy has an elongated shape and is relatively smooth in appearance, with a prominent central bulge that is bright and concentrated. Faint dust lanes are visible on one side, indicating the possibility of a disk component that we are viewing nearly edge-on. There may be a very faint companion or tidal debris on the periphery of the galaxy. The light from the galaxy appears to be redshifted, suggesting it is relatively distant. The galaxy's structure suggests a stable, relatively evolved system, possibly in the process of transitioning from a spiral to an elliptical morphology.
