The galaxy exhibits a flattened, disk-like morphology, appearing nearly edge-on from our vantage point. There is a noticeable central bulge, though its prominence appears relatively small compared to the overall disk size. Diffuse spiral arm structures are suspected, although difficult to resolve given the nearly edge-on presentation. The light distribution suggests active star formation. There is no obvious indication of a strong bar structure. No significant signs of ongoing major merging events or tidal disturbances are noted within the limitations of this image. Overall, the galaxy appears to be a spiral galaxy with ongoing moderate star formation and a relatively small bulge.
