The galaxy appears as a relatively smooth, elliptical-like structure. Its overall color profile suggests a population of older stars, based on the redder hue of the object, and the absence of readily distinguishable spiral arms. The galaxy appears moderately bright, potentially indicative of a large stellar population. There is a slight hint of a more irregular or disturbed morphology. However, this may also be due to the limitations of image resolution. Overall, the galaxy presents as a mature, quiescent system, possibly an elliptical galaxy with little current star formation.
