The galaxy presents a primarily smooth morphology, suggesting an elliptical or lenticular type. The overall shape appears mostly round, with a slight deviation towards an intermediate form, but it is not elongated. There is no strong evidence of ongoing merging events or major disturbances; however, there is a slight chance for minor disturbance that could be present. The galaxy exhibits a strong central concentration of light that gradually fades into the surrounding halo. The color indices suggest the presence of a relatively old stellar population, with minimal ongoing star formation. Overall, this galaxy appears to be a massive, evolved system.
