The galaxy appears as a relatively compact object, exhibiting a smooth light distribution with a slightly elliptical shape. The color suggests a moderate population of evolved stars, potentially indicating ongoing or recent star formation activity. There are no readily apparent spiral arms or a distinct disk structure, which, coupled with the high smoothness fraction, suggests it may be an elliptical or lenticular galaxy, or a spiral galaxy seen face-on with poorly defined spiral arms. There are no obvious signs of major mergers or strong tidal disturbances. The overall impression is that of a mature galaxy undergoing relatively quiescent evolution.
