The galaxy presents an elliptical or lenticular morphology. A notable, luminous central bulge dominates the galaxy's structure. Faint disk like features can be seen surrounding the bulge. Spiral arms are faintly visible around the disk. The colour suggests an aging stellar population and low dust content. The size of the bulge dominates the galaxy. There are no signs of a major disturbance, suggesting the galaxy has experienced no major merging activity recently. The galaxy's overall appearance is relatively smooth.
