The galaxy presents as a spiral type, viewed at an oblique angle. The disk component dominates the overall structure, exhibiting a faint but discernible spiral arm morphology. These arms appear somewhat patchy, with a clumpy distribution of light. A central bulge is evident, though not particularly prominent, displaying a smooth, concentrated luminosity. The overall color index suggests ongoing star formation, particularly in the spiral arms, indicated by their bluer hue compared to the redder bulge component. There is a moderate degree of dust obscuration visible, giving the galaxy a slightly mottled appearance. The axial ratio indicates a flattened shape. There is no evidence of a significant tidal disturbance or interaction with a nearby galaxy based on the image data.
