The galaxy presents as a centrally concentrated object with a generally elliptical morphology, although not perfectly spherical. Its light profile appears smooth, lacking prominent spiral arms or irregular features. The color gradient suggests a population of older stars, more concentrated towards the center, with a slightly bluer hue observed in the surrounding regions, indicative of some ongoing star formation or a younger stellar population in these areas. There is some minor visual disturbance of its shape; however, it mostly presents a relaxed structure. The galaxy displays a modest angular size on the image, implying it is relatively distant. Overall, this galaxy is likely a luminous, massive system undergoing a transition from active star formation to a more quiescent phase of evolution.
