The galaxy presents a flattened, disk-like morphology, viewed at an oblique angle. A central bulge is clearly visible, appearing bright and concentrated. Faint spiral arm structures emanate from the central bulge. These arms are not well-defined and appear somewhat flocculent, with varying degrees of stellar density. The overall color of the galaxy is yellowish-white, indicative of an older stellar population, though some bluer regions are apparent within one of the spiral arms. The galaxy exhibits a moderate degree of rotational symmetry. There is no obvious evidence of recent major merger activity or tidal disturbances.