The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright, yellowish-orange hue, which fades gradually towards the outer edges. There is a subtle elongation evident, suggesting a deviation from a perfectly circular shape. Minimal discernible dust lanes or spiral arm structures are observed. Faint reddish tinges are apparent in the galactic halo. The galaxy appears relatively undisturbed, with no major signs of tidal interactions or ongoing mergers. The dominant light likely originates from an older stellar population. The galaxy is relatively massive. The star formation rate is relatively low.