The galaxy presents as a spiral type, though the spiral arms are somewhat indistinct. The central bulge exhibits a yellowish hue, suggesting an older stellar population. A flattened disk surrounds the bulge, viewed at a slight angle. Patches of bluer light are observed within the disk, potentially indicating regions of active star formation. Some reddish areas are also present, possibly indicating dust lanes or regions of evolved stars. The galaxy's overall form is not perfectly circular; it appears somewhat elongated along one axis, with some degree of disturbance observed that could be the sign of an interaction with another galaxy or merger, but this could also be the result of internal processes.
