The galaxy appears to be a spiral galaxy, seen nearly edge-on. The disk structure is evident, although somewhat obscured. There is a noticeable dust lane running along the major axis, bisecting the galaxy and contributing to its apparent redness. The bulge appears relatively small and indistinct, not dominating the overall light profile. There is evidence of disturbed morphology, potentially suggesting a minor interaction or merger in its past, or ongoing. The galaxy shows hints of active star formation.

