The galaxy presents a largely smooth and diffuse light distribution, suggesting a dominant spheroidal component. There is a hint of a slightly elongated shape. The central region exhibits a brighter, concentrated core. Faint blueish extensions are slightly visible in the periphery, potentially indicative of faint spiral arms or tidal features. The overall color appears relatively red, suggesting an older stellar population and lower ongoing star formation activity. There may be some minor disturbances or interactions visible in the outer regions.
