The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. The galaxy's core exhibits a bright yellowish-white hue, suggestive of an older stellar population. There is a slight elongation of the overall structure, though it is largely round. There is no clear evidence of spiral arms or distinct dust lanes. The light smoothly diminishes with increasing distance from the core, showing no clear disturbances or signs of recent major mergers.
