The galaxy presents a generally smooth morphology, with a high degree of central concentration. There is no readily discernible spiral structure or distinct disk component. The object appears largely spheroidal with a degree of ellipticity, deviating slightly from a perfect circle. Color gradients suggest a stellar population that is somewhat more evolved than the galaxy's periphery, trending towards redder hues at the core and a slightly bluer and less bright extended envelope. There are no strong indications of recent or ongoing major mergers or significant tidal disturbances, though subtle asymmetries in the outer regions cannot be entirely ruled out. Overall, the galaxy appears to be a relatively massive system with a moderate rate of star formation.
