The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in luminosity outwards from the core. The overall shape deviates slightly from perfectly circular, exhibiting a somewhat elongated, cigar-like appearance. There is a hint of bluer light within the central region, suggesting the presence of a younger stellar population, potentially indicating ongoing or recent star formation activity. No prominent spiral arms or distinct features like dust lanes are apparent. There is no visually obvious evidence of a major merger or significant tidal disturbance.
