The galaxy exhibits a morphology suggestive of a spiral galaxy viewed at an oblique angle. A central bulge is discernible, appearing somewhat elongated along the major axis. The disk component shows evidence of spiral arm structure, albeit somewhat indistinct. There appears to be a substantial degree of disturbance in the morphology, potentially indicating an ongoing or recent merger event. Faint tidal features may be present, extending outwards from the main galactic body. The color profile indicates ongoing star formation, particularly in the spiral arms. The nucleus appears relatively quiescent.
