The galaxy presents as a somewhat distorted spiral, though possessing a considerable smooth central bulge. The bulge exhibits a yellowish-white hue, suggesting an older stellar population with relatively low ongoing star formation. Fainter spiral arms are discernible extending from the central bulge. The arms appear somewhat patchy, indicating regions of localized star formation, though they are not sharply defined. These regions display a bluer tint. The overall shape deviates slightly from a perfect spiral structure, possibly exhibiting signs of a minor gravitational disturbance or interaction. No large-scale tidal tails or obvious signs of an ongoing major merger are visible, but subtle asymmetries in the arm structure hint at a potential past interaction. The galaxy has an estimated effective radius, or half-light radius, of just over 4 kiloparsecs, giving it an angular size of roughly 2 arcseconds.
