The galaxy presents as a flattened, disk-like structure, likely viewed at a moderate inclination. A central bulge is apparent, exhibiting a somewhat smooth morphology. The disk component shows evidence of spiral arm structure, although it appears somewhat flocculent rather than grand design. The color profile suggests active star formation, particularly within the disk, indicated by the bluish hue. Overall, the galaxy exhibits characteristics intermediate between a pure elliptical and a late-type spiral, appearing as an intermediate spiral or possibly a lenticular galaxy with ongoing star formation. There is a hint of minor tidal disturbance or interaction in the disk, but it is not a major merger event.