The galaxy presents a largely smooth, elliptical morphology with a concentrated central bulge. The core region displays a yellowish hue, suggesting an older stellar population dominated by redder giants and dwarfs. Fainter, diffuse extensions are visible, transitioning to a bluer color in the outer regions. The round shape indicates a minimal degree of rotational support. No obvious spiral arms or dust lanes are discernible within the image's resolution and color depth. Subtle irregularities or disturbances in the outer halo may indicate recent or ongoing minor merger events. The galaxy appears relatively isolated, showing no obvious signs of strong gravitational interaction with other nearby galaxies. Star formation may be present, but is likely weak.
