The galaxy presents a largely smooth morphology, lacking discernible spiral arms or a prominent central bar. It appears elliptical in shape, exhibiting a near-circular profile with a slight elongation. The light distribution suggests a concentrated central bulge that gradually fades outward. The color gradient indicates a redder hue in the central regions transitioning to slightly bluer tones in the outer areas, indicating a potential difference in stellar populations, with older stars dominating the core and younger stars more prevalent in the outskirts. There are no obvious signs of recent or ongoing major mergers or tidal disturbances.
