The galaxy appears as a centrally concentrated, elliptical-like object with a smooth light distribution. There is no obvious spiral structure. The galaxy exhibits a dominant yellow-orange hue, suggesting an older stellar population. There are no visible dust lanes or distinct star-forming regions, indicating low star formation activity. The overall morphology suggests an early-type galaxy, potentially an elliptical or lenticular galaxy seen at a distance. There is no evidence of tidal features or major disturbances that might indicate a recent merger event, although a minor disturbance cannot be ruled out based on the image alone. The galaxy's round shape reinforces its early-type classification.
