The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely elliptical, with a high degree of roundness observed in its shape. There is a possible indication of a very weak disk. The light distribution suggests a single central bulge, without evidence of a bar or spiral arm structure. A subtle color gradient is present, exhibiting a slightly bluer hue towards the outer regions. The galaxy does not display any signs of major mergers or significant tidal disturbances.
