The galaxy presents as a relatively smooth, elongated structure with a high degree of central concentration. The primary color distribution indicates an older stellar population, with a dominant yellowish-white hue throughout the galaxy. Subtle blue colors are present throughout the galactic structure. These colors may be due to the existence of hot, young stars that are still forming. Faint irregular areas of color are present, which indicates the presence of small amounts of recent or ongoing star formation activity within the disk. There is no obvious spiral structure or bar visible, and the galaxy appears relatively undisturbed with no signs of a recent major merger. Overall, the morphology is consistent with that of a disk galaxy that has evolved significantly.
