The galaxy presents an elliptical morphology, appearing largely smooth and featureless. Its light profile exhibits a centrally concentrated bulge, characterized by a yellowish-white hue suggesting an older stellar population. The overall shape is noticeably elongated, with an axis ratio indicating a significant departure from circularity. There is a subtle color gradient moving outwards from the core, transitioning towards a slightly redder, fainter halo, indicative of a broader distribution of stars. The overall structure suggests an evolved system, likely devoid of significant ongoing star formation in the core. The overall impression is of a galaxy in a relatively quiescent state.
