The galaxy presents as an elongated, cigar-shaped structure. The light distribution appears relatively smooth and centrally concentrated. The core displays a yellowish hue, suggesting an older stellar population. There is a slight gradient towards bluer colors in the outer regions, hinting at the presence of younger stars, though not in significant quantities. There are no obvious spiral arm structures or dust lanes visible. The galaxy shows a slight asymmetry, and hints of disturbance in the surrounding region, but does not appear to be undergoing a major merger.
