The galaxy exhibits a roughly elliptical morphology. A bright, concentrated central bulge is clearly visible, suggesting a significant stellar density in the galactic nucleus. The galaxy is not perfectly smooth in appearance. Evidence for disturbances may be present due to the non-uniform color and texture throughout the galaxy. These disturbances do not appear to be major, suggesting that if merging is occurring, it is a minor disturbance, not a complete major merger. The primary color observed is in the blue-green spectrum. The galaxy displays an overall moderate angular size, not appearing particularly compact nor excessively extended. 
