This galaxy presents as an edge-on disk galaxy. It exhibits a prominent central bulge with a slightly boxy appearance and a relatively high degree of central concentration. The disk itself appears smooth, with no immediately discernible spiral arm structure. There is little evidence of ongoing major merger activity or significant tidal disturbances. Color gradients suggest a possible distribution of stellar populations, with the bulge exhibiting a yellower, possibly older stellar population, while the outer regions of the disk may contain bluer, younger stars indicating some active star formation. The galaxy shows significant dust lane activity obscuring the central bulge.
