The galaxy appears to be a relatively smooth, elliptical galaxy. It is characterized by a bright, concentrated central bulge, surrounded by a more diffuse halo. The light distribution within the galaxy suggests an older stellar population. The galaxy displays a fairly round morphology with no obvious signs of spiral arm structure or significant tidal disturbances, potentially indicating a lack of recent major mergers. The color gradient appears to transition from a slightly bluer hue in the outer regions to redder in the core, which is generally expected for this galaxy type.
