The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. There is a somewhat elongated, elliptical shape to the galaxy. The central region exhibits a bright, compact core, indicative of a high concentration of stars. The galaxy displays a color gradient, transitioning from a slightly bluer hue in the immediate vicinity of the core to a redder color in the outer regions. This color variation suggests a possible difference in stellar populations or dust content between the central and outer areas. There are some subtle irregularities present in the outer regions of the galaxy, potentially hinting at minor disturbances. Overall, the galaxy seems to be a relatively undisturbed system.
