The galaxy appears to be a spiral galaxy, observed at an oblique angle. The galactic bulge appears bright with a slight orange hue, indicating an older stellar population, potentially with less ongoing star formation. A flattened galactic disk extends from the bulge. The disk presents a greenish tint, which could signify a modest amount of ongoing star formation, although this is difficult to assert definitively given the oblique viewing angle. The galaxy has a mostly smooth and regular structure with no obvious signs of major mergers or tidal disturbances, although some minor asymmetry could be present in the outer disk region. The galaxy possesses a relatively compact structure.
