The galaxy presents as a somewhat elongated, cigar-shaped structure. It exhibits a disk-like appearance with some evidence of internal features, though the overall impression is relatively smooth. There appears to be a possible tidal tail or minor disturbance visible in the morphology, though the galaxy appears to be generally isolated, with no major signs of a large ongoing merger. The color profile is moderate, indicating an actively star-forming population, with some areas appearing distinctly bluer.
