The galaxy presents as a face-on spiral with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Spiral arms are clearly visible, though they appear somewhat tightly wound. The arms display a bluer color, indicative of ongoing star formation. Dust lanes are subtly visible, tracing the inner edges of some spiral arms. There is no evidence of a strong central bar structure. The overall appearance indicates a galaxy of substantial mass, actively forming stars, and possessing a well-defined spiral structure with a relatively prominent bulge. There is no indication of a major merger event, though some minor tidal disturbances cannot be ruled out.
