This galaxy exhibits a generally smooth, elliptical morphology. The light distribution is centrally concentrated with a core that appears a yellowish-orange hue, suggesting an older stellar population dominating the central region. Moving outwards from the core, the galaxy exhibits a more diffuse halo with faint blue-ish tones, possibly indicating the presence of some younger stars or ongoing, albeit low-level, star formation. The galaxy appears elongated, with a cigar-like shape, deviating moderately from a perfectly circular form. There are no obvious signs of major tidal disturbances or ongoing mergers. The overall structure suggests a relatively undisturbed system that is transitioning away from active star formation, toward a more quiescent state.
