The galaxy presents an elliptical morphology. It appears largely featureless, with a smooth light distribution lacking prominent spiral arms or a distinct bar structure. There is a concentrated central bulge with a high degree of sphericity, surrounded by a more diffuse halo. The color profile suggests an older stellar population, as indicated by the yellowish-orange hue, which may indicate a reduced amount of on-going star formation. There is a slight asymmetry in the outer regions. No apparent dust lanes or signs of recent major merger events are visible.
