The object presents as a galaxy at a moderate redshift. It appears relatively smooth and lacks strong spiral arm features, suggesting a classification leaning towards elliptical or lenticular. The light distribution is centrally concentrated, with a gradual decrease in surface brightness towards the outer edges. There is a slight elongation, but it is mostly round. There are no clear signs of a major ongoing merger, although some minor disturbances cannot be ruled out at this resolution. The color profile indicates a population of older stars, contributing to its yellow-orange hue. The galaxy's overall morphology is consistent with an early-type galaxy that may have a relatively low star formation rate.
