The galaxy displays a complex morphology, potentially indicative of an ongoing or recent interaction. The main body exhibits a smooth, somewhat elliptical profile, with a bright, concentrated core region. Emerging from this core is a fainter, elongated structure that extends away from the main body. This structure shows signs of tidal disruption, suggesting gravitational interaction with another galaxy. There appears to be a separate region of enhanced brightness along this tidal feature. The color gradients across the galaxy indicate a population of older stars in the smoother core, while the tidal feature might host younger, bluer stars due to triggered star formation resulting from the interaction. Overall, the galaxy appears to be in a dynamically active state.
