The galaxy presents a generally smooth, elliptical morphology. Its light profile appears concentrated towards the center, with a gradual decrease in intensity outwards. The central region exhibits a yellowish hue, possibly indicating an older stellar population. Faint, diffuse extensions surround the core, showing hints of bluer colors in the outer regions, suggesting the presence of younger stars, but this is not definitive. There is no prominent evidence of spiral arms or a distinct disk structure. Minor asymmetries or disturbances are not clearly visible, suggesting a relatively quiescent state. Overall, the galaxy appears to be a relatively isolated and evolved system.
