The galaxy presents a generally smooth, elliptical morphology. It displays a centrally concentrated bulge region that graduates smoothly outward. The color profile indicates a generally older stellar population, particularly concentrated in the core. There is a hint of a disk structure with the galaxy appearing somewhat elongated. The disk exhibits some subtle blue tones indicating ongoing, yet subdued, star formation. No major disturbances or merging features are readily apparent in the image, suggesting a relatively isolated system, possibly with minor ongoing interactions.
