The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a near-circular profile, with no obvious strong deviations from rotational symmetry. The core region presents a bright, yellowish-white appearance, suggesting a high concentration of older stellar populations. Surrounding the core, the galactic disk displays a bluer hue, indicative of younger, hotter stars and potentially ongoing star formation. The galaxy shows only minor disturbances, with no prominent tidal tails or obvious signs of an ongoing major merger event. Overall, it presents the characteristics of a relatively undisturbed galaxy undergoing moderate star formation.
