The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elongated, rounded morphology. The core exhibits a bright, yellow-white color, which suggests a concentration of older stars. The outer regions of the galaxy display a gradual decrease in luminosity and a subtle shift towards redder hues. There is no distinct spiral arm structure or prominent dust lane visible in the image, indicating it is most likely an elliptical galaxy. There may be a small disturbance visible in the light emanating from the galaxy, possibly the early stages of a merger with a small dwarf galaxy.
