The galaxy appears to be an elliptical galaxy with a generally smooth morphology. It presents a centrally concentrated light profile with a gradual decrease in luminosity outward from the core. The galaxy exhibits a yellowish color, suggestive of an older stellar population and relatively low current star formation rate. No distinct spiral arm structures or significant dust lanes are discernible, indicating that it is likely a fairly evolved system. The shape appears relatively round. There is no visual evidence of major merger activity or significant tidal disturbances in the immediate vicinity of the galaxy.
