The galaxy presents a largely smooth, elliptical morphology. The light distribution is centrally concentrated with a gradual decrease in intensity outwards, indicating a spheroidal structure. The core exhibits a yellowish hue, which might be due to an older stellar population. There is minimal evidence of spiral arm structures or significant dust lanes. It appears quite regular and lacks major disturbances in its overall form. There is some bluer light outside of the core suggesting star formation is occurring but the galaxy's red color suggests the star formation rate is relatively low.
