The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology. The light distribution suggests an older stellar population, indicated by the yellowish-orange hue concentrated in the central bulge. The galaxy possesses an elongated shape. There is no evidence of spiral arms, dust lanes, or active star formation regions visible in the image. The galaxy appears to be isolated, without any obvious signs of tidal interactions or ongoing mergers. It seems to be a relatively undisturbed system.
