The galaxy presents as an elliptical morphology, appearing largely smooth and rounded, with minimal discernible features such as spiral arms or a prominent disk structure. The light distribution appears concentrated toward the center, indicating a high degree of central mass concentration. The galaxy displays a color gradient, shifting from a bluer hue in the outer regions to a redder hue in the core. This color gradient could indicate a difference in stellar populations, with the central bulge composed of older, redder stars, while the outer regions contain younger, bluer stars with lower metallicity. The object appears undisturbed, without visual signs of recent major mergers or tidal interactions. Faint irregular disturbances may be present.
