The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. There appears to be a subtle color gradient, with the core exhibiting a slightly yellower or golden hue, suggestive of an older stellar population. The outer regions display a gradual fading of intensity, but lack discernible spiral arms or distinct features. The galaxy appears largely undisturbed with no obvious signs of a major merger event. It is most likely a relatively massive galaxy, with low ongoing star formation. The galaxy shows a moderate degree of ellipticity.
