The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region displays a yellowish-orange hue, suggestive of an older stellar population. The galaxy's overall shape is somewhat elongated. Faint hints of a disk structure are perceptible extending from each side. No obvious spiral arms or dust lanes are discernible within the image. There is very slight color variation across the surface of the galaxy. The galaxy appears relatively isolated, with no signs of ongoing merger activity or significant tidal disturbances in its immediate vicinity.
