The galaxy presents a generally elliptical morphology, appearing largely smooth and centrally concentrated. The core exhibits a bright, yellowish-orange hue, suggesting an older stellar population dominating the central region. There is a subtle color gradient, with the outer regions appearing somewhat bluer, hinting at the possibility of more recent, albeit limited, star formation activity relative to the core. The galaxy does not display any prominent spiral arm structures or significant dust lanes. No major disturbances such as tidal tails or distorted morphology are immediately apparent, suggesting the absence of recent major merger events. The galaxy appears relatively isolated, with no obvious signs of interaction with nearby galaxies in this field of view. It's overall shape is close to round.
