The galaxy presents as a smooth, elliptical morphology, with a high degree of central concentration. The core region appears bright and yellowish-white, possibly indicating an older stellar population. A fainter, more diffuse halo surrounds the core, extending along the major axis of the ellipse. Subtle color gradients are observable from the core outwards, shifting toward a slightly bluer hue in the outer regions. No distinct spiral arm structures or obvious dust lanes are discernible, suggesting a relatively quiescent galaxy with a low star formation rate. The overall form is highly rounded, exhibiting minimal deviations from a perfect ellipse. There appear to be very minor disturbances, but no major mergers seem to be occurring. The galaxy appears to be fairly massive.
