The galaxy presents as an elliptical or lenticular system, observed nearly edge-on. There's a smooth, centrally concentrated bulge, displaying a distinct yellowish hue, suggesting an older stellar population. A flattened disk component is present, but the lack of resolved spiral arms or distinct dust lanes indicates a relatively quiescent system, potentially with minimal ongoing star formation. The outer regions of the disk fade gradually, forming an envelope around the central bulge. Overall, the galaxy appears well-defined and relatively undisturbed.