This galaxy presents as a moderately luminous, elliptical or lenticular system. It exhibits a smooth, centrally concentrated light profile with a discernible bulge. There is a subtle color gradient, shifting from a slightly bluer hue in the outer regions to a redder tint toward the nucleus. No obvious spiral arm structures or dust lanes are observed. The overall shape appears somewhat elongated, potentially indicating a minor degree of tidal disturbance or a slightly barred structure, though this is not definitively visible. Based on its red color, we can estimate that it is likely a massive galaxy with a low star formation rate. 
