The galaxy presents as a relatively smooth object with a slightly elliptical morphology. There is a subtle hint of a disk-like structure, although it's not sharply defined. The galaxy exhibits a color gradient, appearing bluer towards the center and gradually becoming redder in the outer regions. This color distribution suggests a higher concentration of younger, hotter stars in the central region and a population of older, cooler stars further out. There are no signs of strong tidal features or major disturbances that would indicate a recent or ongoing major merger event, though there are minor visual irregularities. Overall, the galaxy appears relatively undisturbed.
