The galaxy presents as a single, concentrated body with an elliptical or spheroidal morphology. There is a high degree of central concentration with no discernible spiral arms or bar-like structures. Its color appears to be dominated by yellow or orange hues, suggesting an older stellar population with minimal ongoing star formation. The galaxy exhibits a high degree of smoothness, implying a well-mixed stellar population with no signs of significant dust lanes or recent mergers. The overall form is undisturbed, with no tidal tails, bridges, or other morphological irregularities that would indicate recent interaction with another galaxy.
