The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The light distribution is centrally concentrated, with a bright core that gradually fades into the outer regions. There is no obvious dust lane or any significant signs of ongoing mergers or tidal disturbances, and the galaxy appears to be isolated. Color gradients are subtle, the central region appearing slightly yellower than the outer regions, which exhibit a redder hue. Overall, the galaxy appears to be a relatively undisturbed elliptical galaxy with a moderately high mass and a low star formation rate.
