The galaxy appears to be a relatively luminous, early-type system at a redshift indicating a moderate distance. The morphology is largely smooth and elliptical in shape, with a high degree of central concentration. The color profile shows a general trend of a redder hue, indicative of an older stellar population. There are slight disturbances, and it is possible that the object is undergoing a minor merging event with a smaller galaxy. The object appears to be relatively large, indicating a significant stellar mass. Although difficult to tell, the lack of any clear spiral arms suggests that it's a non-star-forming galaxy.
