The galaxy exhibits a smooth, elongated morphology, appearing cigar-shaped. There is a central bulge region that appears brighter than the surrounding area. The color gradients within the galaxy suggest a population of older stars concentrated in the bulge, grading into bluer, younger stars toward the outer regions. Faint spiral arm structures may be present, though they are poorly defined and somewhat disturbed, or potentially a disk galaxy. Overall, the galaxy's structure suggests it may be undergoing, or have undergone, some past interaction or disturbance. The galaxy shows no strong evidence of ongoing major mergers but does present some minor asymmetries or perturbations.