The galaxy presents a generally smooth, elliptical morphology. The core region exhibits a high degree of luminosity, appearing as a concentrated, bright, yellowish-orange hue, indicative of an older stellar population with fewer hot, young stars. There is a slight elongation visible, which could imply either a disk component viewed at an angle or the result of a past or ongoing gravitational interaction. Evident are potential disturbances in the outer regions of the galaxy, which could be indicative of a potential merger with another galaxy. There is some subtle blueish light present in the outskirts.
