The galaxy presents as an edge-on spiral, exhibiting a relatively smooth morphology with a prominent central bulge. The bulge appears rounded and tapers into a faint, extended disk. The dust lane typically associated with edge-on spiral galaxies is not sharply defined but is suggested through some color variance in the dust of the disk. Little evidence of active star formation is readily apparent. The galaxy appears relatively isolated, with no major signs of tidal disturbances or recent merger events.
