The galaxy presents as a relatively compact, disk-like structure viewed at an angle. It exhibits a smooth, centrally concentrated light distribution, indicating a prominent bulge component. Some asymmetry can be discerned, suggesting potential minor disturbances within the galaxy's structure, but no obvious signs of a major merger or strong tidal interactions are present.

The galaxy displays a color gradient, with a yellowish-white core and a bluer outer disk, which indicates active star formation.
