The galaxy presents as a relatively smooth, centrally concentrated object, appearing elliptical in shape. A yellowish hue dominates its overall color, suggesting an older stellar population with a lower rate of ongoing star formation. No distinct spiral arms or prominent dust lanes are visible, which further supports the impression of a morphologically early-type galaxy. The object's light is primarily composed of redder wavelengths, which could be a factor of its distance. There is no presence of tidal tails or distortions, which indicates a lack of recent major mergers.