The galaxy presents a generally smooth, elliptical morphology. It appears to be a centrally concentrated system, with a radial color gradient indicating a potentially older stellar population in the core and younger population towards the outer regions. The absence of distinct spiral arms or a prominent disk suggests it is likely an elliptical galaxy, with a high degree of radial symmetry. There is a faint hint of bluer hues towards the periphery, which may indicate ongoing star formation. There is no obvious sign of dust lanes or tidal features that would suggest a recent merger event or significant interaction with another galaxy. It appears to be a relatively undisturbed system.
