The galaxy presents a smooth, elliptical morphology. Its core region exhibits a high degree of light concentration, appearing bright and slightly yellowish. Progressing outward from the core, the light intensity gradually diminishes. The outer regions display a bluer hue, possibly indicating some younger stellar populations or ongoing star formation at a low rate. There are no prominent spiral arms or other distinct features discernible, and there is no obvious sign of it being actively involved in a major merger. However, there is some evidence of a possible minor disturbance visible in the indistinct shape of the galaxy. The roundness is relatively oblate in shape.
