The galaxy presents as a slightly elongated, elliptical structure. The central bulge appears bright and yellowish, potentially indicating a population of older stars. Moving outward from the core, a bluer and fainter disk-like component is observed. This outer region likely hosts a younger stellar population and possibly ongoing star formation. There is only a hint of spiral structure, it is either not a spiral galaxy or the spiral arms are very tightly wound or diffuse. The overall morphology suggests a galaxy in transition, possibly evolving from a more active, star-forming phase to a more quiescent state. There is no apparent major interaction or merger occurring. The galaxy appears relatively undisturbed.
