The galaxy presents a largely smooth, elliptical morphology. It appears well-resolved and rather compact. The color profile suggests a population of older stars, and the galaxy exhibits a spherical shape. The light is concentrated toward the core, with a gradual falloff in intensity towards the edges. There is some evidence of minor disturbances, but the overall structure remains largely undisturbed. The lack of distinct spiral arms indicates a lower rate of current star formation activity.
