The galaxy presents as a relatively smooth, elliptical structure. Its core exhibits a concentrated, bright emission, which fades gradually towards its outer regions. The overall color profile suggests an older stellar population, with a discernible lack of strong blue emission indicative of recent or ongoing star formation. There is very little evidence of spiral arms or significant dust lanes and minimal features or disturbances. It appears to be an isolated galaxy, without any noticeable signs of interaction or merging events occurring.