The galaxy presents a largely smooth and centrally concentrated morphology. The light distribution appears nearly spheroidal. There is a slight color gradient, with the central region exhibiting a more yellowish-white hue, suggesting an older stellar population compared to the faint, diffuse outskirts which appear slightly bluer. No distinct spiral arms or bar features are discernible. The overall light profile suggests minimal recent merger activity. Based on its visual smoothness and roundness, this galaxy may be an elliptical or lenticular galaxy.
