The galaxy presents as a single, relatively smooth concentration of light. Its morphology appears generally elliptical or spheroidal, with a slight elongation. The color is a yellowish-white, suggesting an older stellar population with fewer hot, young stars, although there may be some bluer regions present. There does not appear to be a distinct disk component, and the galaxy lacks obvious spiral arm structure. No strong tidal features, merging companions, or other significant disturbances are immediately apparent in the image, though a subtle asymmetry may indicate minor interaction. The light profile is centrally concentrated, with a gradual decrease in intensity outwards.
