The galaxy presents as a centrally concentrated, relatively smooth distribution of light. Its morphology is consistent with an elliptical galaxy type, displaying an overall rounded appearance. There is minimal evidence of spiral arms or significant disk features. Color gradients suggest a population of older stars. A faint blue hue can be observed around the core of the galaxy, indicating a relatively low level of recent star formation. The galaxy does not show obvious signs of recent major merger activity or significant tidal disturbances.
