The galaxy presents as a moderately bright object with a smooth, elliptical morphology. The light distribution suggests a central bulge that is approximately circular and quite bright, indicating a high concentration of stars in that region. The galaxy is slightly elongated, appearing somewhat cigar-shaped. There is a subtle color gradient visible, with a yellowish-white core transitioning to a slightly bluer hue in the outer regions, potentially indicating some ongoing star formation, albeit not very pronounced. No distinct spiral arms or significant dust lanes are observed. The galaxy appears relatively undisturbed, lacking strong indications of recent major mergers, although some minor disturbances cannot be ruled out.
