The galaxy appears to be a spiral galaxy, viewed nearly face-on. It exhibits two prominent, loosely wound spiral arms. The arms display a clumpy structure, suggesting active regions of star formation. The central bulge is moderately sized and exhibits a yellowish hue, indicating a population of older stars. A faint bar-like structure might be present, extending through the bulge region. The galaxy demonstrates an overall disk-like morphology. There are no obvious signs of recent major merger activity, however, minor tidal disturbances cannot be ruled out.
