The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a yellowish hue, suggesting an older stellar population. Fainter, bluish extensions are visible at either end of the central bulge. The overall morphology indicates a galaxy that is smooth, rather than having obvious spiral arm structures. The color gradient, from yellow center to bluish outer regions, may reflect differing stellar populations or dust content within the galaxy. The presence of an apparently round, bright, and yellowish object to one side of the main galaxy body could suggest a possible interaction or a star cluster within the galaxy's halo.
