The observed galaxy exhibits a pronounced disk-like morphology, viewed nearly edge-on from our perspective. The central bulge appears relatively prominent and smoothly luminous, displaying a yellowish-orange hue, indicative of an older stellar population. The disk, extending outwards from the bulge, shows a more diffuse and bluer tint, suggesting ongoing or recent star formation activity, although no distinct spiral arm structure is discernible in this image. There may be dust lane obscuration running along the midplane of the disk, based on the slight darkening observed in the image, though further data would be needed to verify its existence and extent. There are no obvious signs of major tidal disturbances or recent mergers.