The galaxy presents as a relatively compact structure with a central region of concentrated luminosity, possibly indicating a bulge. There is a suggestion of disk-like features, but these are not sharply defined. The overall color profile leans towards bluer hues in the central region, and it appears to be smooth in appearance. The red shift indicates it is a distant object, and the lack of well-defined spiral arms or a clear elliptical shape implies it may be either a disturbed system or a lenticular galaxy undergoing transformation. There is a disturbance in the morphology that indicates it could possibly be a merger with another galaxy. Further investigation, including spectroscopic analysis, is required to determine its classification.
