The galaxy exhibits a smooth, elliptical morphology with a high degree of central concentration. The light profile appears to be fairly uniform, lacking prominent spiral arms or distinct features. The galaxy appears to be somewhat elongated. Color gradients are subtle, with a slightly bluer hue in the outer regions and a yellowish-white core, suggesting older stellar populations dominate the central region, while younger stars may be present at the edges. There is no indication of significant dust lanes or active star formation regions visible in this image. There is a hint of minor disturbance but it is not classified as a merger, and the galaxy appears isolated. 
