The galaxy presents a discernible spiral structure. Two distinct spiral arms emanate from the central bulge, winding loosely outward. These arms exhibit a mottled texture, suggesting regions of active star formation interspersed with dust lanes. The central bulge appears moderately sized and has a smooth morphology with a yellow hue, indicative of an older stellar population. A weak bar structure may be present, extending across the bulge along the spiral arms. There are no signs of a major ongoing merger. The outer regions of the galaxy are less defined, with a gradual fading of the spiral arms into the background. The overall color suggests a mixed population of stars, with regions of both younger, bluer stars and older, redder stars.