The galaxy presents a generally smooth morphology, appearing elliptical in shape. The central region exhibits a concentrated, bright core. Moving outward from the core, the light gradually diffuses, suggesting a decreasing stellar density. There are no obvious spiral arm structures or significant dust lanes visible. The overall color appears relatively uniform, tending towards a yellow-white hue, indicative of a population of older stars. Subtle disturbances are not obvious in this view but cannot be ruled out without more advanced imaging.
