The galaxy presents as a relatively smooth and rounded object. The core appears to be a bright, concentrated region of stellar density, exhibiting a warm hue indicative of an older stellar population. Extending outward from this central region is a more diffuse halo of light, showing a slight gradient in color, transitioning toward cooler tones. There appears to be a subtle hint of disc-like morphology, although it is not distinctly resolved. Overall, the galaxy's structure suggests it may be an early-type galaxy, possibly an elliptical, with little evidence of active star formation. Minor disturbances may be present, based on the slight irregular shape in the extended halo of light. The overall appearance indicates a gravitationally stable and relatively quiescent system.
