The galaxy presents as a single, dominant object with a smooth and centrally concentrated light profile. It appears elliptical in shape, tending toward an elongated form rather than perfectly spherical. The central region displays a higher intensity, suggesting a dense nucleus or bulge. Moving outward from the core, the light gradually diminishes with no distinct features like spiral arms or a bar structure readily discernible. The galaxy exhibits a subtle color gradient; the core leans towards a yellow hue, while the outer regions take on a slightly bluer tint, hinting at the presence of younger stellar populations at the fringes. There are no obvious signs of ongoing merger activity or tidal disturbances affecting its overall morphology.
