The galaxy appears to be a relatively compact and smooth system. Its color profile suggests a population of older stars, indicating it is likely an early-type galaxy. The overall shape is somewhat elliptical, appearing nearly round, with a lack of prominent spiral arm structures or a distinct central bulge. There is only a minor disturbance observed, so there is an assumption it is not undergoing any major merging events, or that this galaxy is the result of a merger. The galaxy exhibits a relatively small angular size, suggesting it is at a significant cosmological distance.
