The galaxy presents as a single, luminous object with a smooth and centrally concentrated light profile. The galaxy exhibits an elliptical morphology, appearing moderately rounded. It displays a noticeable color gradient, transitioning from a bright, yellowish core to fainter, reddish outskirts. There is no discernible evidence of spiral arms, a disk, or recent major merger activity. Minor irregularities or distortions are not apparent, suggesting a dynamically relaxed system. The galaxy's smooth morphology suggests a relatively old stellar population. The overall color profile indicates a relatively low star formation rate and a high mass.
