The galaxy appears as a well-defined elliptical structure, exhibiting a smooth, centrally concentrated light distribution. The morphology suggests an evolved system, consistent with a relatively quiescent state. The color gradient reveals a central region with a yellowish-white hue, likely indicative of an older stellar population. Fainter bluish-green emissions are present in the surrounding area, potentially tracing regions of more recent, though limited, star formation. No prominent spiral arms or dust lanes are discernible, reinforcing the classification as an elliptical type galaxy. Overall, the galaxy exhibits a coherent structure with a modest color variation suggesting a diverse stellar population within a relatively mature system. There appears to be very little, if any, ongoing merger activity, and its shape suggests that it is not a particularly flattened elliptical.
