The galaxy presents as a relatively compact and moderately luminous system with an elliptical morphology. It exhibits a smooth, diffuse light distribution, indicating a predominantly older stellar population. The color index suggests a redder, more evolved system. There's no discernible spiral structure or active star-forming regions visible. It seems the galaxy is not currently undergoing any major merger events, although it might be experiencing minor tidal interactions, as indicated by some subtle disturbances in its outer regions.
