The galaxy presents a prominent spiral structure. Two well-defined spiral arms emanate from a bright, centralized bulge. These arms are relatively extensive and exhibit a somewhat flocculent morphology, without a high degree of symmetry. They are moderately wound. The central bulge appears yellowish, suggesting an older stellar population. The spiral arms show bluer regions, likely indicating areas of active star formation. The galaxy appears relatively isolated, without obvious signs of major tidal disturbances or ongoing mergers, though subtle asymmetries are present within the disk. The disk is not edge-on. A faint, extended halo is subtly visible.
