The galaxy exhibits a flattened, disk-like morphology, with a central bulge that appears relatively smooth. The disk appears tilted, with a near edge-on orientation, indicating a relatively low probability that it is a face-on spiral galaxy. The light distribution suggests that the galaxy is characterized by a smooth distribution of stars, and is more likely to be an early-type spiral or lenticular galaxy. There appear to be some minor disturbances in the galaxy, as seen by some variations in the light, so it is possible the galaxy underwent a minor merger or other type of disturbance.
