The galaxy presents as a flattened, elongated structure, consistent with a disk-like morphology viewed at an oblique angle. The central region exhibits a higher surface brightness and a yellowish-orange hue, possibly indicating an older stellar population and dust obscuration. Fainter, bluer regions are observed in the outer parts of the disk, suggesting younger stars and ongoing star formation. The galaxy appears relatively smooth, with no obvious spiral arm structures or signs of significant disturbances such as tidal tails or prominent dust lanes. It has a cigar shape and does not appear to be undergoing any major mergers with other galactic structures.
