The galaxy appears as a centrally concentrated object with a relatively smooth morphology. It presents an elliptical shape with a significant intermediate axial ratio, not perfectly round, nor particularly elongated. There are faint indications of a possible disc structure, but it is not particularly prominent. The galaxy appears to be a relatively massive system with suppressed star formation activity. The core of the galaxy appears to have a yellow-reddish hue suggesting a relatively old stellar population. The light from the galaxy appears to be consistent with a system at a redshift of approximately 0.35, suggesting it is at an intermediate distance. Signs of any ongoing merger events or major disturbances are not readily apparent.
