This galaxy appears to be a relatively smooth, elliptical galaxy. The light is concentrated towards the center with a radial decrease in surface brightness. The galaxy exhibits an overall orange-red hue, suggesting an older stellar population, with limited ongoing star formation. The shape is close to round, without any strong signs of spiral arm structure or a prominent disk. There is no obvious presence of dust lanes or other irregular features. There are no strong indications of recent or ongoing major merger activity; the galaxy appears relatively undisturbed. The overall morphology suggests a mature system.
