The galaxy appears to be an elliptical or lenticular galaxy at moderate redshift. It presents a relatively smooth morphology with a high degree of central concentration. Some blue light emanates from distinct areas around the galaxy, indicating possible low-level star formation regions. There is little evidence of spiral arms or a well-defined disk structure. No ongoing major merging activity or significant tidal disturbances are observed. The overall color suggests a population of older stars, but with some recent or ongoing star formation. The galaxy's shape is close to round.
