The galaxy presents as a largely smooth, centrally concentrated object. Its morphology appears elliptical, with a high degree of roundness. The central region exhibits a pronounced brightness and yellowish hue, suggesting an older stellar population. There is a smooth transition from the core outwards. The galaxy's light profile indicates minimal presence of distinct features such as spiral arms or a prominent disk. There might be some minor disturbances in the galaxy's structure, but it is likely not undergoing a major merger event. The estimated size based on half-light radius suggests it's a moderately sized galaxy. The overall color suggests a population of stars with relatively little recent star formation.
