The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, displaying a somewhat spheroidal structure with a hint of asymmetry. Color gradients suggest a possible age gradient in the stellar populations, with a yellowish hue concentrated towards the core, potentially indicating an older stellar population, and a bluer halo. The galaxy lacks a clear spiral arm structure or prominent dust lanes, which strengthens the elliptical classification. There may be evidence of a very faint and diffuse disk. No signs of major mergers or tidal disturbances are evident in the image. 
