The galaxy presents as a largely featureless elliptical or lenticular form. It exhibits a smooth, concentrated central bulge that dominates the overall luminosity. The halo fades gradually from the core. The core appears to be relatively red in color, possibly indicating an older stellar population with minimal ongoing star formation. There is a slight hint of a flattened disk. There are no signs of spiral arms or significant dust lanes visible in this image. There may be a faint distortion visible that can be seen as minor disturbances. The morphology suggests a galaxy that has either completed or is approaching the end of its major star-forming epoch.
