The galaxy presents an overall elliptical morphology, appearing elongated in shape. The central region exhibits a bright, concentrated luminosity, likely indicative of a dense stellar population and possibly a central supermassive black hole. Progressing outward from the core, the luminosity gradually decreases. There are no discernible spiral arm structures or significant dust lanes visible in this image. The galaxy appears relatively smooth in texture, with only subtle variations in color and brightness across its extent. The overall color of the galaxy appears somewhat redder in the center, grading to a slightly bluer hue toward the edges, which may indicate ongoing, albeit modest, star formation in the outer regions compared to an older stellar population dominating the central bulge. The overall structure suggests a galaxy that has undergone significant evolution, potentially a transition from a spiral morphology to a more elliptical form. There are no immediate indications of any recent major merger events, although minor disturbances cannot be ruled out based solely on this image. The shape deviates from a perfect circle, leaning more toward a cigar-like appearance.
