The galaxy presents a smooth, elliptical morphology, with a high degree of central concentration. The light profile exhibits a noticeable color gradient, shifting from a yellowish-white core to a redder halo. This suggests an older stellar population dominating the central region, with relatively less recent star formation. The galaxy displays a slight elongation, deviating minimally from a perfectly circular form. The outer regions are diffuse, indicating a gradual decline in stellar density with increasing radius. There's no visual evidence of strong spiral arm structures or significant dust lanes. Overall, the galaxy appears as a relatively quiescent system.
