The galaxy presents as a single, relatively smooth structure with a high degree of central concentration. It exhibits a near-spherical morphology. The central region displays a bright, concentrated luminosity, characterized by a yellowish-orange hue, suggesting a population of older stars. The outer regions display some color variation, though not indicative of clearly resolved structures. The galaxy appears to be relatively isolated, showing no signs of major ongoing interactions or mergers. There are no obvious spiral arm features or a defined disk component evident in this image, which seems to be an elliptical galaxy. It exhibits a subtle gradient in surface brightness from the core outwards.
