The galaxy appears to be a relatively smooth, elliptical galaxy with a dominant central bulge. Its overall shape is moderately round, showing minimal signs of distortion or tidal features. The light distribution suggests a concentration of older stellar populations, indicated by the yellowish hue dominating the central region. There is a slight color gradient, with the outermost regions appearing marginally bluer, which could indicate the presence of younger stars, though not very many. There is no obvious dust lane or spiral arm structure detectable in the image. There is also no visual sign of any interaction with a nearby galaxy. The galaxy seems well-defined, with a gradual decline in light intensity towards its outer edges, indicating a smooth transition into the background sky.
