The galaxy presents a largely smooth, elliptical morphology. Its central region exhibits a bright, concentrated core with a yellowish-orange hue, indicative of an older stellar population. Moving outward from the center, the color gradient suggests a decreasing concentration of older stars and a subtle shift towards bluer wavelengths. This hints at the presence of some younger stars in the outer regions, although not to a significant degree. There is a slight asymmetry to the galaxy's outer regions, perhaps indicating that there was a minor merger event in the past. However, the galaxy appears largely undisturbed.
