The galaxy presents as a relatively compact, centrally concentrated object. Its overall morphology appears smooth, with a high degree of symmetry and no obvious spiral arm structure or significant tidal features indicative of recent major merger activity. The light profile suggests a dominant bulge component. Color gradients appear minimal, and the galaxy seems to be homogenous. There is no distinctive blue color, suggesting that the object is composed of older stars. The galaxy exhibits a roundness that is nearly circular.
