This galaxy exhibits a flattened, disk-like morphology seen edge-on. A central bulge appears present, characterized by a concentration of light that is brightest in the center and diminishes outwards. Extending horizontally from the central bulge, a faint and elongated structure consistent with a galactic disk is observed. There are suggestions of possible distortions or tidal features, specifically one elongated structure on one side, perhaps a faint tidal tail. The light distribution across the disk is irregular, which suggests a system that is undergoing or has undergone some form of disturbance. The galaxy possesses a low surface brightness compared to the surrounding sky, and the redder color in the central regions might indicate an older stellar population in the bulge, whilst blue hints on the disk’s edge suggest regions of more active star formation.
