The galaxy presents a moderate level of structural complexity. A central bulge region is prominent, exhibiting a relatively smooth texture and a somewhat concentrated luminosity. The overall color of this central region leans toward the redder end of the spectrum.

Surrounding the bulge, there is evidence of a disk component. This is visible as a fainter, more diffuse structure extending outwards from the core. There appears to be a slight asymmetry to the disk. The disk is not uniformly colored; there are hints of bluer regions interspersed within it, possibly indicating areas of more active star formation. These bluer patches are not distinctly resolved. The overall appearance does not suggest a grand design spiral structure, but rather a more flocculent or irregular form. There may be an interaction or disturbance occurring, although this is not definitive based on the imagery.
