The galaxy presents as a centrally concentrated, elliptical morphology with a smooth, largely featureless appearance. The core is characterized by a bright, yellowish-orange hue, suggesting a population of older stars and/or significant dust obscuration. The luminosity appears to decrease gradually from the core outwards. There is no clear evidence of spiral arms or a prominent disk structure. Faint blue tinges are seen at the very edges. The galaxy appears undisturbed, with no signs of recent major mergers or tidal disruptions.
