The galaxy appears to be a disk galaxy, viewed nearly edge-on. The central bulge is prominent and elongated along the major axis, exhibiting a roughly rounded profile. There are indications of a flattened disk structure extending outward from the bulge. The disk displays a subtle blueish tint, particularly at the edges. The galaxy appears relatively undisturbed with no obvious signs of major mergers or tidal disruptions, though there may be some minor asymmetries or disturbances in the disk's outer regions. It displays a smooth appearance, with limited distinct star-forming regions visible in this image. The color gradient suggests older stellar populations dominate in the central bulge while younger stars may be more prevalent in the disk, indicating ongoing star formation.
