The galaxy presents a generally smooth and elliptical morphology, with a high degree of central concentration. The light profile indicates a centrally bright core that diffuses outward, transitioning from a reddish hue at the nucleus to a more greenish-yellow color in the outer regions. No distinct spiral arms or bar structures are discernible. There is no obvious evidence of strong tidal interactions or ongoing major mergers, although subtle asymmetries or minor disturbances may be present. The overall structure suggests a relatively evolved system with a potentially older stellar population dominating the central regions, while some younger star formation may be occurring in the outer disk.
