The galaxy presents a disk-like morphology, exhibiting prominent spiral arm structures. The arms appear relatively tightly wound. A substantial central bulge is observed, contributing significantly to the overall luminosity. A bar structure seems to bisect the bulge, extending into the inner spiral arms. The color distribution indicates the presence of both older stellar populations in the bulge, indicated by the yellowish hue, and younger, bluer stars within the spiral arms, possibly indicative of ongoing star formation. There appears to be a higher density of these blue stars in the spiral arms, contrasting with the smoother yellow color in the bulge. There do not appear to be any merging galaxies associated.
