The galaxy presents as a centrally concentrated, lenticular or early-type spiral form. It exhibits a smooth, diffuse light profile, suggesting a dominant bulge component with little active star formation. The galaxy appears more elongated than circular but not significantly so. There may be a hint of a faint disk structure, but it is subtle. There is no evidence of recent major merger activity, though the presence of some mild irregularities in the outer regions can not be excluded from the image. The galaxy possesses an intermediate mass, and low star formation rate.
