The galaxy presents as a flattened, disk-like structure, viewed at a significant inclination. The central region exhibits a bright, concentrated bulge, characterized by a yellowish-white hue. The disk component surrounding the bulge shows a bluer color, with a smooth texture. There is an apparent absence of distinct spiral arm structures. The outer edges of the galaxy appear diffuse, fading into the background sky. The smooth morphology suggests a lack of recent major merger activity. The color gradient, shifting from redder hues in the bulge to bluer tones in the disk, suggests differing stellar populations and ongoing star formation. A slight asymmetry may be present, but this could be due to the angle that the galaxy is observed at.
