This galaxy presents a relatively smooth, elliptical morphology. It displays a notable color gradient, transitioning from a bluer hue in its northwestern sector to a redder, more golden tone towards the southeastern side. This color variation suggests a potential difference in stellar populations across the galaxy, with the bluer region potentially indicating a zone of more recent or ongoing star formation activity. The redder region likely contains older, redder stellar populations. There might be some minor disturbances present, which may be due to an ongoing or past merger event. The galaxy appears moderately compact, with a diffuse halo extending beyond its central, brighter region.
