The galaxy appears as a centrally concentrated, elliptical-like structure. Its core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. The light gently diffuses outward from this bright center, transitioning into a more subtle, greenish color in the outer regions. The overall form displays a high degree of smoothness, with no obvious spiral arm structures or large-scale irregularities. The galaxy's shape is elongated, deviating noticeably from a perfect circle. The lack of prominent dust lanes or patches indicates relatively low amounts of interstellar dust. No significant signs of recent major merger events are visible, though slight disturbances or minor tidal features cannot be entirely ruled out at this resolution.
