The galaxy presents as a spiral galaxy with a defined disk structure. Its appearance is dominated by its spiral arms, which exhibit a tightly wound morphology. The central bulge is relatively small and does not dominate the overall galactic structure. The galaxy displays a blue hue, particularly noticeable in the spiral arms, indicative of active star formation regions. The overall color suggests a population of young, hot stars contributing significantly to its luminosity. The spiral arm count is difficult to discern due to the angle and image resolution. There are no obvious signs of a major ongoing merger event. The disk is seen at an angle, showing some disk structure. The galaxy's apparent size suggests it is a moderately sized galaxy.
