The galaxy presents as a centrally concentrated elliptical or lenticular system, with a high degree of symmetry and smoothness. It is generally round in appearance, lacking any prominent spiral arm structures or strong morphological disturbances. There appears to be a higher concentration of luminosity near the center, decreasing smoothly outward. A faint hint of extended emission or a very diffuse halo is present around the main body of the galaxy, suggesting a moderate size. There is another small object close to the galaxy; it is uncertain whether this object is interacting with the galaxy or is another galaxy nearby. The galaxy exhibits a moderate redshift, indicating it is relatively distant.
