The observed galaxy presents an elliptical morphology, appearing as a relatively compact object with a smooth, centrally concentrated light distribution. There is little discernible structure, such as spiral arms or a prominent disk. The galaxy exhibits a subtle color gradient, with the central region appearing marginally redder compared to the outer regions. The overall color suggests a population of older stars. There is no apparent active galactic nucleus or starburst activity indicated by bright, point-like emission or irregular features. Marginal features appear to indicate minor disturbances in the galaxy morphology.
