The galaxy presents a largely smooth morphology, with a high degree of central concentration. There is a slight elongation of the galaxy along a discernable axis, though its overall shape is close to being round. I can detect a hint of color variation across the galaxy’s structure. The central region appears to be slightly more yellow or gold in color than the outer regions, which appear a more pale blue. This may indicate an older stellar population concentrated in the bulge, with a younger stellar population in the outer disk. The appearance is largely undisturbed, with no clear signs of tidal tails or strong morphological distortions.
