The galaxy presents as a lenticular or possibly a spiral galaxy seen at a high inclination, nearing edge-on. The central bulge is prominent, exhibiting a concentrated, smooth light distribution, appearing yellowish-white. The disk is relatively faint and elongated, extending significantly further than the bulge. Hints of spiral structure are discernible, though not sharply defined, manifesting as subtle color variations within the disk; these variations may be due to the angle and dust extinction, and possible traces of underlying spiral arms. The overall morphology suggests a substantial stellar mass, with ongoing but potentially moderate star formation activity within the disk. There is a hint of some tidal disturbance or minor interaction, which would support a star formation rate that is elevated.
