The galaxy presents a flattened, elliptical morphology. It exhibits a smooth, featureless appearance across its visible structure, with a notable absence of prominent spiral arms or distinct star-forming regions. The central bulge appears bright and concentrated, transitioning smoothly into a more diffuse disk. Color gradients are observed, with the core region displaying a yellowish-orange hue, suggestive of an older stellar population. Fainter blue tones are subtly distributed throughout the outer disk, possibly indicating the presence of some younger stars. The galaxy's orientation is such that we observe it at a significant inclination angle. There is no obvious sign of interaction or merging with another galaxy. The overall structure suggests a system dominated by an evolved stellar population with a relatively low rate of on-going star formation.
