This galaxy presents as an elliptical type, exhibiting a centrally concentrated luminosity profile. The core is a bright yellowish-white, suggesting an older stellar population. The galaxy appears largely smooth, lacking any prominent spiral arms or dust lanes. There is a subtle transition in color outward from the core to a bluer hue, indicating the potential presence of some younger, bluer stars in the outer regions, which could be regions of low-level star formation. The object possesses a moderate degree of roundness. Overall, there are no signs of any significant ongoing merger activity or major disturbances to its structure.