The galaxy presents as a somewhat elongated, disk-like structure, oriented at an oblique angle relative to our line of sight. The central region exhibits a high degree of luminosity, appearing as a concentrated, bright bulge with a yellowish hue. This suggests a substantial population of older stars within the galactic nucleus. 

Moving outwards from the core, the disk displays a gradual decline in surface brightness. There appears to be a subtle color gradient, with the outer regions of the disk exhibiting a slightly bluer tinge compared to the central bulge. This implies the presence of younger, hotter stars in the spiral arms, although any distinct spiral arm structure is not clearly resolved in this image. The smoothness of the galactic morphology suggests that the system is fairly evolved and not undergoing any major mergers. There may be some minor asymmetry visible in the outer regions of the disk suggesting there might be tidal disturbances.
