The galaxy presents a largely smooth, elliptical morphology. Its core appears bright and concentrated, exhibiting a yellow-orange hue, which may indicate an older stellar population. The outer regions fade gradually into the background, showing hints of a bluer tint. This suggests some ongoing, though possibly subdued, star formation activity within the galaxy. There are no distinct spiral arms or a prominent disk. Minor irregularities are present, and these may be indications of gravitational interactions. The galaxy is generally round in appearance.
