The galaxy presents as a relatively smooth and centrally concentrated elliptical system. It exhibits a high degree of roundness in its overall shape. There is a noticeable absence of distinct features such as spiral arms or a prominent disk structure. The color profile suggests an older stellar population, with a dominant yellowish-orange hue concentrated towards the center of the galaxy. There is little evidence of ongoing major star formation, based on the apparent color and lack of bright blue regions indicative of young, hot stars. The galaxy does not seem to show any obvious signs of recent or ongoing major mergers or tidal disturbances, with a generally undisturbed morphology.
