The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. The light profile suggests a significant spheroidal component. The galaxy displays a yellow-orange hue in its core, possibly indicating an older stellar population dominating the central region. The outer regions exhibit a slightly bluer color, suggesting the presence of younger stars, though the overall color indicates a passively evolving system. There is no apparent spiral structure or evidence of active star formation, and the galaxy's morphology does not show any signs of recent major mergers or significant tidal disturbances. The general rounded shape and lack of obvious features suggest a relaxed, dynamically evolved state.
