The galaxy appears as a fairly smooth, centrally concentrated object. It exhibits an elliptical morphology, approaching circularity. There is a dominant central bulge exhibiting a yellowish hue, suggesting an older stellar population.  There is an absence of apparent spiral arm structure or significant dust lanes, with the overall color profile indicating passive star formation. No signs of major merger events are present, with the general form being largely undisturbed. The galaxy is relatively compact and shows little evidence of extended features.
