The galaxy presents a generally smooth and rounded morphology. Its light distribution appears relatively uniform, lacking prominent spiral arms or a distinct central bulge. The overall color suggests a population of older stars, with a moderate redshift indicating it is a distant object. There is some indication of possible interaction or merger activity, as evidenced by slight disturbances in its otherwise regular structure. The galaxy's estimated size is several kiloparsecs in diameter, suggesting it is a substantial system. Star formation appears to be relatively quiescent.
