The galaxy presents as a largely smooth, centrally concentrated object with a generally elliptical morphology. There is a noticeable radial color gradient, transitioning from a yellowish core to a bluer outer region. No distinct spiral arm structure or prominent dust lanes are apparent. There is the presence of a low-level extended halo of diffuse light. There is no evidence of a major ongoing merger or tidal disruption, though a slight asymmetry in the outer regions cannot be ruled out as evidence of a minor interaction. Overall, the galaxy appears to be a relatively undisturbed system.
