The galaxy presents as a centrally concentrated elliptical type, exhibiting a smooth, symmetrical morphology. The light distribution suggests a spheroidal structure, lacking prominent spiral arms or a distinct disk. The core region is bright and appears relatively compact, indicating a possible high stellar density, with the luminosity fading gradually toward the outer edges. The color is generally yellowish-orange, consistent with an older stellar population and low levels of current star formation, although there is the possibility of the existence of some on-going star formation within the galaxy. There is only a slight indication of any disturbance of the main body of the galaxy.
