The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It exhibits an elliptical shape, leaning towards a more flattened, intermediate form rather than perfectly round or elongated. There is little evidence of significant merger activity or major disturbances in its structure, suggesting a relatively quiescent evolutionary state. The color indices indicate a galaxy dominated by older stellar populations, emitting strongly in the redder bands of the spectrum. It appears as a large, massive galaxy with minimal star formation. 
