The galaxy appears as a relatively smooth, elliptical-like structure. The central region exhibits a bright, concentrated core, suggesting a significant density of stars and possibly a supermassive black hole. The overall shape is elongated, but not highly so, displaying an intermediate roundness. There is little to no evidence of spiral arms or significant dust lanes. The color profile suggests a population of older stars, likely lacking in active star formation. No major disturbances are visible, implying a relatively quiescent state. There is a faint disk structure surrounding the core.
