The galaxy presents an asymmetrical morphology, potentially indicative of an ongoing or recent interaction. One region displays a relatively smooth, concentrated, and luminous core with a slight blueish hue, possibly due to the presence of younger stars. Adjacent to this is a less defined area appearing more diffuse and reddish-orange, which might result from dust obscuration or an older stellar population. There are hints of tidal features or minor disturbances surrounding the main body, further implying gravitational interaction. Overall, the galaxy seems to exhibit a mixture of characteristics, combining a bulge-like central component with possible distortions from external influences.
