The galaxy presents as a slightly tilted disk. The central bulge appears significant and exhibits a yellowish-white hue, suggesting an older stellar population. The disk component is less distinct, with a bluer color gradient extending outwards from the bulge. The galaxy is elongated in shape, possibly due to its viewing angle or intrinsic morphology. There are no readily apparent spiral arm structures or significant dust lanes visible in this image. Overall, the galaxy has a smooth appearance, which suggests it might be an early-type spiral galaxy. 
