The galaxy presents a largely smooth morphology, exhibiting a primarily elliptical shape. There is no clear evidence of spiral arms or a prominent galactic disk. The galaxy appears highly concentrated, with a radial light profile that gradually decreases from its center. There appears to be a minor degree of internal disturbance. There is no distinct nucleus. The galaxy's light distribution is remarkably symmetrical and possesses a high degree of central concentration, suggesting an evolved stellar population.
