This galaxy presents a distinct disk-like morphology. It appears to be a spiral galaxy viewed nearly edge-on. A central bulge is evident, exhibiting a yellowish hue, which might indicate an older stellar population. The disk surrounding the bulge shows a bluer tint, potentially signifying areas of active star formation. There is a subtle indication of spiral arm structure within the disk, though the near edge-on orientation makes it challenging to discern their precise form. The galaxy does not show signs of major disturbances or a recent merger event. Its apparent smoothness suggests it has not experienced significant gravitational interactions recently.
