The galaxy presents a relatively well-defined spiral structure. Two prominent spiral arms extend outwards from a moderately bright central bulge region. These arms appear loosely wound, tracing a somewhat grand design. There is evidence of a bar-like structure bisecting the central bulge, though it seems weakly defined. The color suggests ongoing star formation within the disk, particularly along the spiral arms. The galaxy disk is not precisely edge-on, but shows only a moderate inclination. There are no obvious signs of significant tidal disturbances or major mergers, though subtle asymmetry hints at a potential minor interaction or internal dynamic process. The image resolution is not sufficient to discern detailed star clusters or dust lanes. The bulge appears relatively small compared to the overall size of the disk component.
