The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. The galaxy appears elongated, with a major to minor axis ratio of approximately 0.8. The core region exhibits a bright, concentrated luminosity. The galaxy displays a reddish hue, suggesting an older stellar population and minimal ongoing star formation. There is no evidence of significant tidal features or disturbances, indicating that the galaxy is not currently undergoing a major merger. The overall morphology suggests a relatively evolved system, consistent with an elliptical galaxy type.
