The galaxy appears as a centrally concentrated object with a generally smooth, elliptical morphology. There is little evidence of distinct spiral arms or significant dust lanes. The core region exhibits a bright, yellowish-white color, possibly indicative of an older stellar population. The outer regions fade gradually into the background, suggesting a relatively smooth decline in stellar density with increasing radius. There might be some minor disturbances, or perhaps faint tidal features present, but it is hard to say for sure. Overall, the galaxy seems to be a relatively undisturbed system, likely an elliptical galaxy viewed from a nearly face-on perspective. The color profile suggests relatively low star formation rate.
