The galaxy presents a generally smooth, elliptical morphology. There is a dominant central bulge that gradually fades into the outer regions, which are also fairly homogenous in colour. There is a slight elongation, but overall the shape appears relatively round. The colour suggests that the galaxy is comprised primarily of older stars, implying a low rate of star formation. There is no indication of spiral arms or a prominent disk structure. Furthermore, there are no obvious signs of tidal tails or significant morphological disturbances, indicating that the galaxy is unlikely undergoing a major merger event. There are no distinct dust lanes or regions of active star formation visible in the image.
