The galaxy presents an elliptical morphology, appearing largely smooth and centrally concentrated. The core exhibits a yellowish-white hue, indicating a population of older stars. The galaxy's light profile suggests a relatively high degree of symmetry, with no discernible spiral arm structures or prominent dust lanes. There is a suggestion of a slight elongation, potentially hinting at a mild tidal interaction or an intrinsic aspherical shape. The overall color indices suggest a red sequence galaxy, with low levels of recent star formation activity.
