The galaxy exhibits a distinct disk structure, viewed at an oblique angle, indicating it is likely a spiral galaxy. The spiral arms are prominent and loosely wound, extending outwards from a bright central region. The central bulge appears relatively small or non-existent. There is evidence of two main spiral arms. A possible minor tidal disturbance or interaction may be present, indicated by irregularities or distortions in the spiral arm structure. There is no strong evidence of a central bar feature. The disk appears to have a blue hue, suggesting active star formation.
