The galaxy presents a generally smooth, elliptical morphology. Its color profile suggests a dominant population of older stars, exhibiting a yellowish hue at the core that fades into red at the extremities of the galaxy. The overall shape is largely spheroidal, showing a slight deviation toward being somewhat less than perfectly round. There is minimal evidence of spiral arms or a well-defined disk structure; instead, the light distribution appears relatively even. This galaxy shows no obvious signs of a major ongoing merger event, although a minor disturbance or interaction cannot be ruled out.
