This galaxy presents a flattened, elongated morphology, approximating a cigar shape. Its overall color appears bluish-white, suggesting a moderate presence of younger, hotter stars. The light distribution appears relatively smooth, with no immediately obvious spiral arm structures or a prominent central bulge. There is a slight color gradient from the central region toward the edges, but it is not very distinct. The galaxy appears relatively isolated, with no immediately visible signs of major tidal disturbances or ongoing merger activity. Its integrated light suggests it is a medium mass galaxy, with moderate levels of star formation. It is likely a disk galaxy, possibly a late-type spiral or an irregular galaxy viewed edge-on.
