The galaxy presents as a fairly smooth, elliptical-like structure with a high degree of central concentration. It appears to be relatively featureless, with no distinct spiral arms or bar visible. There is a slight elongation, with the galaxy appearing somewhat oval in shape. The color profile is primarily yellowish-white, suggesting an older stellar population with fewer young, massive stars. There is a subtle color gradient with a slightly redder hue towards the center, possibly indicating a higher concentration of older stars or dust in the core region. The galaxy does not show any obvious signs of recent or ongoing mergers or major disturbances.
