The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. There is minimal evidence of spiral arm features or significant disk structure. The light profile appears relatively uniform, with a gradual decrease in intensity from the core outwards. The color gradient indicates a population of older stars, with a yellowish-red hue dominating the galaxy's overall appearance. There is no clear indication of active star formation regions or substantial dust lanes. The galaxy exhibits a slightly elongated shape, but lacks significant morphological distortions indicating a recent or ongoing merger event. The overall appearance suggests a galaxy that has largely exhausted its gas supply and experienced significant star formation in the past.
