The galaxy appears to be a disk-shaped system, seen nearly edge-on. It is relatively small and exhibits a prominent central bulge. The bulge appears smooth and concentrated. The disk itself is elongated, with a higher concentration of light towards the center. A subtle dust lane may be present obscuring the central plane of the galaxy. The outer regions of the disk are fainter and less defined. The galaxy appears to be largely undisturbed, with no obvious signs of a major merger or tidal interactions, though subtle disturbances cannot be ruled out. The light from the galaxy suggests it is a moderately massive galaxy with a relatively low rate of star formation. The dominant colors observed suggest an older stellar population.
