The galaxy appears to be a relatively smooth, elliptical-like system. It exhibits a concentrated central bulge with a yellowish-white hue, suggesting an older stellar population. The light distribution is quite uniform, with no prominent spiral arms or distinct features visible. There are no clear signs of active star formation or significant dust lanes. The overall shape is nearly circular, with only a slight elongation discernible. It does not show signs of any major disturbances or ongoing merger activity. There may be faint hints of an extended halo, but the data are not conclusive. The galaxy exhibits a consistent color profile from core to edge, implying a well-mixed stellar population.
