The galaxy presents as a moderately luminous, relatively compact system. Its overall form appears elliptical, exhibiting a smooth, centrally concentrated light distribution. The core region is bright and somewhat yellowish or pale orange in hue, which may indicate an older stellar population and a lack of significant recent star formation in the very center. This central region fades gradually into the outer areas, and the light becomes slightly bluer. The isophotes, or lines of equal brightness, suggest a slight elongation of the galaxy, and its light appears uniformly distributed, lacking distinct spiral arms or other well-defined morphological features such as a prominent disk. There's no clear visual indication of active galactic nuclei (AGN) activity based on morphology alone. The galaxy's apparent smoothness suggests it is an early-type galaxy.
