The galaxy presents as a centrally concentrated, relatively smooth structure. It appears elliptical in shape, exhibiting a high degree of roundness. The color profile suggests the presence of a generally older stellar population, with a slight bluish tint. There's no strong evidence of spiral arms or other distinct morphological features typically associated with disk galaxies. There are no clear signs of ongoing major mergers or significant tidal disturbances. A hint of a faint outer halo may be present, though it's poorly defined. The overall appearance is consistent with an elliptical galaxy, likely possessing a substantial stellar mass and a moderate rate of star formation.
