The galaxy presents as a flattened elliptical morphology, with a smooth, diffuse appearance. The core region exhibits a yellowish-white hue, suggesting a population of older stars. Fainter, reddish tendrils extend from the core, possibly indicative of dust lanes or regions of recent, albeit diminished, star formation. A faint, greenish outer halo surrounds the central region. Overall, the galaxy exhibits a relatively quiescent state with little evidence of major disturbances or mergers. The primary structure appears largely undisturbed and relatively homogenous in stellar distribution, although the color variation suggests internal structure and differing stellar populations within the galaxy.
