The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated core. It is generally round in shape, showing no discernible spiral arm structures or significant distortions. The color profile suggests a population dominated by older stars, with a yellowish hue becoming more pronounced towards the galaxy's center. There are no visually apparent signs of active star formation, such as blue knots or HII regions. Based on its overall appearance, this galaxy is likely a quiescent system with minimal ongoing merger activity.
