The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core that fades gradually outwards. There is a lack of distinct spiral arms or prominent dust lanes. The overall color suggests an older stellar population, with a low rate of current star formation. The morphology is generally round with no signs of significant disturbances or ongoing merger activity. The galaxy appears to be a relatively isolated system.
