The galaxy presents as a somewhat elongated, lenticular-like structure. The core exhibits a bright, concentrated luminosity, indicating a substantial stellar density or possibly an active galactic nucleus, though without further spectral analysis, this remains speculative. There is an apparent lack of distinct spiral arm structures, supporting a smoother classification. The color profile suggests a population dominated by older stars. There is a very subtle indication of asymmetry in the outer regions potentially indicative of a minor gravitational disturbance. Overall, the galaxy seems to be a relatively massive system with relatively low star formation rates. The galaxy is likely at a considerable distance, as implied by the redshift.
