The galaxy presents as a centrally concentrated, elliptical-like structure. Its light profile appears smooth, with a high degree of roundness. The core exhibits a yellowish-orange hue, potentially indicating an older stellar population, with a decrease of star formation activity. There is no visible presence of spiral arms or a distinct disk structure. Faint disturbances may be present in the galaxy's outer halo. The estimated size of the galaxy is approximately 10 kpc. Its moderate red shift shows that it is a galaxy that is significantly far away from us.
