The galaxy presents a largely smooth and rounded morphology, suggestive of an elliptical galaxy type, or possibly a lenticular galaxy seen face-on. There is a high degree of central concentration, with brightness decreasing radially outward. The color profile displays a subtle gradient, shifting from bluer hues in the central region to slightly redder tones in the outer parts of the galactic halo. No distinct spiral arm structures or significant dust lanes are discernible. Given the overall color and morphology, the galaxy likely consists of an older stellar population with relatively low current star formation. It shows no signs of any major or minor disturbances that could suggest a recent or ongoing merger.