The galaxy presents as a largely smooth, elliptical-like structure with a concentrated central bulge. Its overall color index suggests an older stellar population, exhibiting a yellowish-orange hue throughout the main body. There are some indications of minor disturbances in its morphology, potentially from past interactions or mergers, though the overall structure remains relatively undisturbed. Its round shape and lack of prominent spiral arms or features indicate it is likely an early-type galaxy, possibly an elliptical or lenticular type. The galaxy appears to be neither undergoing significant star formation nor is it severely disrupted by any major mergers, it is likely in a relatively quiescent state.
