This galaxy presents a peculiar morphology, appearing as a seemingly edge-on system exhibiting a dual structure. It consists of two distinct, bright, and somewhat elongated components aligned along a common axis. Each component displays a bright, central core region, surrounded by a fainter, more diffuse halo or disk. There is some indication of a redder structure associated with the bright components. The overall color appears to be slightly blue-shifted, suggesting active star formation within the galaxy. However, this is dominated by the artifacts of the image. There may be evidence of minor tidal disturbances or faint extensions emerging from the main body of the galaxy, possibly indicative of a past or ongoing interaction. The galaxy appears relatively compact, and the detailed structure of any potential spiral arms or bar features is not readily apparent from this image. The light distribution suggests a complex internal structure, which may require further investigation using higher-resolution observations to fully characterize its nature and evolutionary state. There is a very high probability of this object being an artifact.
