The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated, with a gradual decrease in intensity toward the outer regions. There's a subtle color gradient, with the core appearing somewhat redder compared to the slightly bluer outer regions. No distinct spiral arms or bar structures are discernible. There is no evidence of active galactic nuclei (AGN) in the form of a bright, point-like source at the center. The overall morphology suggests an evolved galaxy, potentially a lenticular or early-type elliptical, with a low rate of on-going star formation. There is no obvious sign of any interaction.
