The galaxy presents as an elliptical structure, elongated along its major axis. The central region exhibits a concentrated, bright core that gradually diminishes in intensity towards the outer edges. The overall color profile indicates a dominance of older stellar populations, evidenced by the yellowish-orange hue in the core. Fainter bluish tinges are present in the outer regions of the disk, but not in well defined spiral arms. There is no prominent spiral structure visible. Slight morphological distortions are observable, suggesting a possible interaction or past merger event.
