The galaxy presents as a relatively smooth, centrally concentrated object with a dominant elliptical morphology. There is little indication of spiral arm structure or a prominent disk. The light distribution appears fairly uniform, with a gradual decrease in brightness from the core to the outer regions. The galaxy appears to be generally round. The color profile indicates a primarily older stellar population, with a yellowish-orange hue throughout. This suggests a lack of significant recent star formation activity across the galaxy. There may be some minor disturbance, but the overall impression is one of a settled, relatively undisturbed system.
