The galaxy presents as a centrally concentrated object with a smooth overall morphology. Its light profile appears relatively uniform, lacking prominent spiral arms or a distinct disk structure. The galaxy exhibits a slightly elongated shape, appearing nearly circular. Color gradients are subtle, with a central region displaying a yellowish hue that fades into a redder component towards the outer edges, suggesting a potentially older stellar population in the galaxy's core. There are no apparent signs of ongoing major merging events or tidal disturbances, and the galaxy seems well-settled. The overall appearance suggests a relatively massive, evolved galaxy with a high Sersic index, which correlates to a low star forming rate.
