The galaxy presents as a largely featureless, elliptical morphology. Its light profile is smooth and concentrated, showing a centrally brightened core that fades outward. The color gradient transitions from a yellowish-white core to a bluish outer halo, suggesting a stellar population that is older toward the center and perhaps younger in the surrounding regions. There is no evidence of spiral arms, bars, or significant dust lanes visible in the image. The overall shape is close to circular in projection. No signs of tidal disturbances or interactions with other galaxies are apparent. Based on the color distribution, the galaxy is likely comprised of a dominant population of older stars, with possibly a small, but non-negligible rate of current star formation.
