The galaxy presents as a relatively smooth, elliptical-like structure. The light is concentrated towards the center, suggesting a prominent galactic bulge. Color gradients suggest an older stellar population, concentrated towards the core. There is a general lack of discernible spiral arm structure or dust lanes indicating that star formation is likely occurring at a low rate. Its profile appears largely undisturbed, lacking significant tidal features or evidence of major mergers. The overall morphology is consistent with an early-type galaxy undergoing passive evolution at a redshift of approximately 0.24.
