The galaxy appears to be a relatively smooth, elliptical galaxy, with an overall rounded morphology. Its core exhibits a bright, concentrated luminosity, suggesting a high stellar density or potential AGN activity. The color profile transitions from a yellowish core to a bluer, less-defined outer region. There's no discernible spiral arm structure or significant dust lanes, which supports its classification as an elliptical galaxy. The lack of significant morphological disturbances indicates the absence of any major recent merger events. Faint extensions are visible around the main body of the galaxy, hinting at a possible extended halo or the presence of tidally stripped material. Overall, the galaxy presents a picture of a mature system that has undergone significant evolution.
