The galaxy appears to be a relatively smooth, elliptical-type galaxy. It exhibits a centrally concentrated light profile, with the luminosity decreasing gradually outward from the core. The core is a bright, yellowish color, suggesting an older stellar population. There is minimal evidence of spiral arms or significant dust lanes within the galaxy, which supports its classification as an elliptical. The overall shape appears close to round, with no obvious elongation or distortion. There are no immediate signs of tidal interactions or major disturbances, indicating a relatively isolated system. Based on the color and morphology, it is likely a massive galaxy with a relatively low rate of current star formation.
