The galaxy presents as a well-defined spiral galaxy with a clearly visible disk structure. Two dominant spiral arms emanate from the central bulge region, displaying a medium winding. The arms appear relatively continuous, showing some patchiness possibly due to differing stellar densities or dust lane presence. The central bulge appears moderate in size and brightness. A bar feature appears to extend through the bulge region, with medium strength. The disk is viewed at an angle where it is close to face on. There are no indications of major merging events, however there might be some minor disturbances. The color profile suggests active star formation within the spiral arms. The galaxy is not particularly compact, showing a diffuse outer region.
