The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a generally round morphology, with minimal visible structure such as spiral arms or prominent dust lanes. There might be a faint and subtle, very small disk that is difficult to observe in this image. The galaxy’s color profile suggests a mature stellar population, potentially dominated by older, redder stars. There are no obvious signs of major ongoing mergers or tidal disturbances, though there is a small chance of minor disturbances. It is a pretty typical galaxy for its estimated mass. The galaxy is somewhat bright, even at its distance.
