The galaxy presents as a centrally concentrated object, displaying a largely smooth morphology. It appears nearly circular in shape. The central region exhibits a bright, concentrated luminosity, suggesting a relatively dense core. The surrounding regions show a gradual decrease in brightness, fading into the background sky. There is little evidence of spiral arm structures or prominent disk features within the image. The overall color profile indicates a possible presence of older stellar populations dominating the light emission. There are no visually apparent signs of ongoing major merger activity or significant tidal disturbances.
