The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is largely spheroidal with a hint of slight elongation, but generally well-rounded. The light profile suggests a dominant bulge component, with a smooth and diffuse stellar distribution. There is no strong evidence of spiral arm structure or a well-defined disk. The galaxy presents with a color gradient, appearing slightly bluer in the central region, indicating younger stellar populations or ongoing star formation. The outer regions seem redder, potentially indicating older, more evolved stars. There is a very slight asymmetry, with a subtle extension or tidal feature on one side.
