The galaxy presents a generally smooth, elliptical morphology. Its light is centrally concentrated, with a bright, yellowish core. The isophotes appear mostly regular and concentric, though there are some subtle irregularities in the outer regions. The galaxy does not display prominent spiral arms or a distinct disk structure. Overall, the light profile suggests an evolved stellar population, with possible ongoing low levels of star formation. There is some subtle asymmetry, possibly due to minor interactions. The galaxy does not show any signs of strong tidal features or a recent major merger event.
