The galaxy presents as an elliptical morphology with a prominent central bulge that is bright and appears yellow-orange in color, indicating an older stellar population. The galaxy exhibits a smooth, diffuse outer envelope. There is a slight elongation, suggesting a deviation from perfect sphericity. There is a small hint of bluer color towards the edges, likely due to younger stars forming, but overall the galaxy is relatively quiescent. No obvious spiral arm structures or significant dust lanes are detected. There are no tidal tails or other clear indicators of ongoing or recent major merger events. The galaxy’s stellar mass is substantial. The central bulge appears to be the dominant feature.
