The galaxy presents as a centrally concentrated object with a generally elliptical morphology. The core exhibits a bright, yellowish-white hue suggesting an older stellar population, potentially a supermassive black hole. Proceeding outward from the core, the light gradually diffuses into a less luminous halo. The halo's coloration subtly shifts towards redder tones, possibly indicative of dust obscuration or a change in stellar populations. The shape of the galaxy is elongated, with a ratio of major to minor axes that is around 3:1, suggesting a relatively flat elliptical form. The texture appears smooth and without discernable spiral arm structures. Overall, the galaxy appears undisturbed, exhibiting no signs of major merger activity. The absence of prominent blue regions suggests a lower rate of ongoing star formation relative to other galaxies.
