The galaxy presents a distinct spiral structure. Two prominent spiral arms are clearly visible, extending from a central bulge. The arms display a moderate winding pattern, not tightly wound but also not loosely defined. The central bulge appears relatively small compared to the overall size of the disk. Within the disk, there are signs of a bar-like feature crossing the central region, though it does not appear to be intensely prominent. There appears to be some irregularity in the outer regions of the disk, possibly indicating a minor gravitational interaction.
