The galaxy presents as an elliptical structure with a smooth, concentrated central bulge. Its overall shape appears elongated, approaching a cigar-like morphology. The galaxy exhibits a color gradient, transitioning from a brighter, yellowish core to a dimmer, redder outer region. There is no discernible spiral arm structure or significant dust lane obscuration visible in this image. No signs of major mergers or tidal disturbances are obvious, although subtle distortions in the outer halo cannot be ruled out based on this image alone. The smooth and centrally concentrated morphology, alongside the color profile, suggests a relatively evolved system, with potentially quenched star formation in the central regions.
