The galaxy presents a predominantly elliptical morphology with a smooth light distribution. The core region exhibits a bright, concentrated luminosity profile that appears relatively homogeneous across the available bands. There is a subtle color gradient moving outwards from the core, where it shifts from a yellowish color to a redder hue at the edges. It shows little to no indication of spiral arm structures or prominent dust lanes, which further supports its classification as an elliptical galaxy. There appear to be no signs of any major mergers or violent disturbances, and no signs of active star formation. Its overall visual texture implies an evolved stellar population.
