The galaxy exhibits a pronounced disk-like morphology, seen at a moderate inclination angle. The central bulge is bright and appears relatively smooth, exhibiting a concentrated luminosity profile. Moving outward from the bulge, the disk shows evidence of spiral arm structures, although they are not sharply defined. There is a bluer color gradient in the outer regions of the disk, suggesting ongoing star formation. The overall structure hints at a late-type spiral galaxy, possibly of the Sb or Sc classification, though it is not definitively barred. No obvious signs of a major ongoing merger are present, but the disk displays some irregularities, perhaps indicative of minor interactions. The size of the galaxy appears relatively moderate compared to other galaxies in the survey.
