The galaxy appears as a centrally concentrated object with a relatively smooth morphology. It presents an overall elliptical shape, although not perfectly spherical. There's a subtle elongation, but it doesn't appear as a highly flattened disk galaxy. There is a slight blue tint to the core, suggesting the presence of some younger, hotter stars, but the overall color is more characteristic of older stellar populations. No prominent spiral arm structures or dust lanes are discernible in the image. There is a faint hint of possible disturbance or tidal features, though it is not conclusive from this image alone. The galaxy does not appear to be undergoing a major merger, though minor interactions cannot be ruled out based solely on this visual data.
