The galaxy presents a distinct spiral morphology. The spiral arms are tightly wound, indicative of a possible grand-design spiral structure, though definitive arm tracing is somewhat obscured. A prominent central bulge is visible, though it appears relatively small compared to the overall disk size. The disk exhibits a generally smooth appearance with blue tinted regions, suggestive of regions of active star formation. Dust lanes appear faint, and indistinct. No obvious signs of major mergers are apparent, though a possible tidal feature suggests minor past interactions or disturbances. A weak bar structure is also indicated by the elongated nature of the central bulge and the slight asymmetry in the inner spiral arms.
