The galaxy presents as a largely featureless elliptical morphology. It exhibits a high degree of central concentration with a smooth, diffuse light distribution that gradually decreases in intensity from the core outwards. No distinct spiral arms, bars, or dust lanes are discernible within its structure. The overall color appears yellowish-red, which may indicate an older stellar population dominated by red giant stars and a relatively low rate of ongoing star formation. The isophotes are generally rounded, with only a hint of ellipticity. There are no obvious signs of recent major merger events or tidal disturbances in its immediate vicinity. The galaxy appears relatively isolated and undisturbed.
