The object appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated, spheroidal morphology with no discernible spiral arm structure. Its color gradient suggests a redder core, potentially indicative of an older stellar population. There are no apparent signs of ongoing major mergers or significant tidal disturbances. Faint, diffuse light extends outwards from the central region, hinting at a more extended halo component. The galaxy's overall smoothness points to a lack of significant recent star formation activity.
