The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The central region exhibits a bright, yellowish-white hue, suggesting an older stellar population and a lack of significant ongoing star formation. A fainter, bluer halo surrounds the core, possibly indicating a younger population of stars or some residual star formation activity. The galaxy appears largely undisturbed, lacking any obvious signs of major merging or tidal interactions. Overall, the galaxy appears to be an elliptical galaxy undergoing a period of quiescence in star formation. Some minor disturbance within the galaxy cannot be ruled out, but there is no strong indication of mergers.
