The galaxy presents a disk-like morphology, viewed at a high inclination. The central bulge appears relatively smooth, and displays a yellowish-orange hue. Surrounding the bulge is a flattened disk with discernible features. The disk exhibits spiral arm structures, though they are not sharply defined. The overall color of the disk suggests the presence of younger stellar populations, perhaps indicative of ongoing, although not vigorous, star formation. There may be a minor disturbance to the galaxy’s structure, such as tidal tails or slightly asymmetrical features, but this is not conclusive.
