The galaxy presents as an elliptical morphology with a high degree of central concentration. Its color profile is predominantly yellow, suggesting an older stellar population and a low rate of ongoing star formation. The galaxy appears relatively smooth, lacking prominent spiral arms or distinct features indicative of recent mergers or interactions, though there is a slight irregular shape to it. A subtle reddish hue is observed toward the lower edge, potentially indicating the presence of dust or a small region of ionized gas. The overall appearance suggests a well-evolved system, possibly a lenticular or elliptical galaxy, with a substantial stellar mass. The overall structure is largely undisturbed, implying a period of relative quiescence in its evolutionary history.
