The galaxy presents as a spiral type, observed at a redshift indicating a significant distance. It exhibits a central bulge with a yellow-orange hue, suggesting a population of older stars. The surrounding disk appears relatively smooth, with hints of blueish regions indicative of younger star formation. The galaxy's morphology leans toward an intermediate state between elliptical and highly-structured spiral, showing subtle, faint arm structures. The overall shape is somewhat elongated. There appears to be some minor disturbance within its morphology, but it doesn't appear to be in the process of a major merger with another galaxy. The galaxy does not appear to have a very high rate of star formation. It has a fairly high mass.