The galaxy appears to be a spiral galaxy, viewed at a moderate angle, not quite edge-on, but significantly inclined. The central bulge is prominent, exhibiting a yellowish-white color, suggesting an older stellar population. The spiral arms are somewhat indistinct and appear relatively tightly wound. Faint bluish regions are observed within the spiral arms, indicating areas of recent star formation. The overall structure of the disk shows some irregularities, possibly suggesting minor gravitational interactions, but no significant tidal tails or distortions are apparent. There is no clear evidence of a prominent dust lane. The galaxy is relatively compact in size.
