The galaxy presents as a relatively compact object with a disk-like morphology. The main body appears to be structured in a fashion with a hint of features. Although these features are apparent, there is also a smooth component. Faint features can be seen that could possibly be signs of disturbance. However, it appears that the object is fairly stable, and a major merger event seems unlikely.

The distribution of light within the galaxy suggests a moderate amount of activity. The central region presents a subtle increase in light intensity and is slightly redder in color.
