The galaxy presents a generally elliptical morphology, appearing relatively smooth with a centrally concentrated light profile. The core is bright and appears yellowish, indicative of an older stellar population dominating its composition. The galaxy exhibits a noticeable color gradient, transitioning from a warmer hue in the core to cooler, slightly redder tones in its outer regions. There are no clearly defined spiral arms or other distinct features readily apparent in the image, which further supports its classification as an elliptical galaxy. The overall structure is compact and lacks significant signs of ongoing star formation. No strong tidal features or merger remnants are visible in the immediate vicinity, suggesting a gravitationally settled system.
