The galaxy appears as a single, moderately elongated object. Its light profile suggests a smooth, but not perfectly spherical, distribution, leaning towards a cigar-like shape. There is a hint of a central concentration, though not a distinct, bright nucleus. The color is predominantly yellowish-orange, possibly indicating an older stellar population. No prominent spiral arms or dust lanes are discernible in the image. There is a slight asymmetry, suggesting possible minor disturbances, though no clear signs of a major merger are evident.
