The galaxy presents an intermediate morphology, appearing neither entirely smooth nor dominated by a clear spiral or elliptical structure. There is faint blueness, indicating some ongoing star formation. Visual inspection reveals possible minor disturbances or asymmetries in the outer regions of the galaxy's disk, suggesting a recent or ongoing minor interaction or merger event. The galaxy's color index indicates it is not a very old, red population, but not as young and actively star forming as the bluest systems. Overall, it appears to be a disk galaxy viewed at an angle, with a substantial bulge.
