The galaxy presents a distinct spiral morphology. Two well-defined spiral arms emanate from a moderately sized central bulge. The winding of the spiral arms appears intermediate, neither tightly wound nor exceptionally loose. Traces of a possible bar structure appear to extend through the central bulge along the major axis. No signs of recent or ongoing major merger events are apparent. Faint, diffuse extensions are visible, suggesting possible interactions or minor tidal disturbances. The color distribution indicates active star formation within the spiral arms, with bluer regions contrasting with the redder bulge.
