The galaxy presents as a relatively smooth, centrally concentrated object with a yellowish-white hue. It exhibits a morphology consistent with an elliptical galaxy, showing minimal signs of spiral arm structures or significant dust lanes. The galaxy appears approximately round in shape, with a subtle elongation that does not classify it as a cigar-shaped galaxy. There is no visually apparent major or minor disturbance, and the galaxy appears to be in a relatively isolated state, with no obvious signs of recent or ongoing merger activity. The core region appears to be the brightest part of the galaxy, and the color suggests older stellar populations dominate.
