The galaxy presents as a concentrated elliptical object. It exhibits a smooth, centrally concentrated light profile. The galaxy appears generally rounded, with no obvious spiral arms or bar structure. The color gradient suggests a redder core, possibly indicating an older stellar population, that is slightly brighter and more luminous than its surrounding area. The outer regions display a subtle color shift towards bluer hues. There is no obvious indication of tidal disturbances or ongoing major mergers in this image, however there is the presence of some minor disturbances or the possibility of a past merger event that has reached a point of relative equilibrium. This system is likely a large and massive galaxy. Overall, this galaxy appears to be a relatively relaxed system.
