The galaxy exhibits a clear spiral structure, with a central bulge that appears moderately bright and concentrated. Two prominent spiral arms emanate from the central region, winding loosely around the galactic disk. These arms display variations in luminosity, potentially indicative of differing stellar populations or dust lane presence. The galactic disk appears relatively smooth, with a slight inclination relative to the observer's line of sight. There is no obvious sign of tidal tails or distortions, which suggests it is relatively undisturbed. The overall color profile suggests a mix of evolved stars in the bulge and younger, bluer stars within the spiral arms, indicative of ongoing star formation.
