This galaxy appears to be a relatively smooth, elliptical-like structure. The central region exhibits a concentrated, bright, yellowish-orange hue, suggesting an older stellar population. The outer regions are more diffuse and exhibit a bluer tint, possibly indicating the presence of some younger stars, but the overall color suggests star formation is not dominant. There is no clear evidence of a spiral arm structure, bar, or ongoing major merger event. The galaxy’s shape is somewhat elongated, showing a deviation from a perfect sphere. There may be evidence of a very minor disturbance in the outer regions of the galaxy, but this is not clear. Overall, the galaxy appears to be a well-formed system, likely in the later stages of its evolution.
