The galaxy presents a primarily smooth morphology, with a concentrated central region exhibiting a reddish-orange hue, suggestive of an older stellar population. A fainter, somewhat bluer halo surrounds the core, indicating the presence of some younger stars or ongoing star formation. The galaxy appears largely spheroidal in shape, although a slight elongation is noticeable. There are no distinct spiral arms or bar structures discernible within the resolution of the image. The overall structure suggests a galaxy that has largely completed its major merging history, appearing relatively undisturbed with no obvious tidal features or signs of recent major interactions.
