The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, diffuse light profile with no apparent spiral arm structure. The central region is brighter and appears yellowish, suggesting a concentration of older stellar populations. Moving outward from the core, the light gradually fades into a faint, extended halo. There is a slight reddish hue observed in one section of the outer region, possibly indicating an area of ongoing, though relatively subdued, star formation or dust absorption. The overall shape appears slightly elongated rather than perfectly spherical. There's no visual evidence of significant tidal disturbances or active galactic nuclei activity based on this single image.
