The galaxy presents a generally smooth and elliptical morphology. The core region exhibits a bright, concentrated luminosity, suggesting a high stellar density. The light profile gradually diminishes outward from the core, lacking any distinct spiral arm structures or prominent dust lanes. There is a very subtle blueish hue present in the outer regions. The color gradient from the core to the outer regions is continuous, indicating a generally uniform stellar population distribution. There are no obvious signs of recent or ongoing major mergers.
