The galaxy presents a primarily smooth morphology, exhibiting a concentrated, rounded structure. The core appears as a bright, yellowish-white, suggesting a significant population of older stars. Surrounding the core, there is a slightly elongated halo with subtle color variations. A faint reddish hue is observed on one side of the galaxy, potentially indicative of dust or regions of on-going star formation, though this is not immediately obvious from the image. A very slight disturbance or asymmetry in the outer regions might suggest a minor interaction with another galaxy in the past, though the overall structure remains largely undisturbed. The galaxy's smooth and centralized light distribution implies an evolved system with a high degree of internal order.
