The galaxy presents as a relatively smooth, elliptical-like structure. There is a central concentration of light, suggesting a prominent galactic nucleus. The overall color appears to be a yellow-orange hue, indicative of an older stellar population with fewer young, massive stars. No distinct spiral arms or bar features are discernible. The edges of the galaxy fade gradually into the background, without sharp delineations, giving a sense of a diffuse stellar halo surrounding the main body. There are no obvious signs of recent major merger activity or tidal disturbances.
