The galaxy presents a generally smooth morphology, although there are some features suggesting disturbances. It is somewhat elliptical in shape, deviating from a perfect circle. The core is bright and concentrated, surrounded by a less luminous and more diffuse halo. There may be some evidence of faint tidal features, potentially indicating past or ongoing interactions with another galaxy or gravitational influences. The galaxy exhibits a blue hue, especially in the core region, suggesting the presence of a population of younger, hotter stars, yet there are redder regions that suggest slightly older populations or increased dust content. There is a hint of a possible merger or significant perturbation occurring, potentially influencing its shape and star formation rate.
