The galaxy presents as a spiral, characterized by well-defined spiral arms emanating from a central bulge. These arms exhibit a tightly wound morphology. The galaxy displays a blue-white hue, suggesting the presence of younger, hotter stars within the spiral arms, consistent with ongoing star formation. The central bulge appears more yellow-orange, indicating a population of older, cooler stars. The galaxy exhibits a high degree of rotational symmetry. There are no prominent signs of tidal disruption or interaction with nearby galaxies, suggesting it is relatively isolated. The galaxy has a small bulge relative to its disk. There appears to be a weak bar structure within the center of the galaxy. The light distribution appears relatively smooth.
