The galaxy presents a somewhat amorphous structure. It exhibits a predominantly smooth appearance with hints of features indicative of either a disk-like component or possible disturbances within the galaxy's morphology. The central region demonstrates higher surface brightness, suggesting a concentrated stellar population or active galactic nucleus. The overall shape tends towards roundness, with a slight deviation towards an elliptical form. There are no prominent spiral arms or a well-defined bar structure discernible. There is a suggestion of minor interaction with another galaxy or an internal disturbance causing some visible asymmetry and irregularity. Overall, it could be categorized as possibly undergoing a merging event, or having a more irregular shape because of internal forces. The color indicates the presence of relatively young, hot stars, and potentially ionized gas. The relatively small angular size in the image suggests this galaxy may be at a considerable distance.
