The galaxy presents as a moderately luminous, reddish-gold elliptical or lenticular-type galaxy. Its light profile appears smooth and centrally concentrated, suggesting an older stellar population with little ongoing star formation. The galaxy's shape is elongated, with a clear departure from perfect circularity. Faint blue tinges are present in the extended halo, which may suggest a more distributed population of stars or the potential for low-level star formation. No apparent spiral arm structure, dust lanes, or signs of active galactic nuclei are immediately discernible from the image. There is little indication of any major merger event.
