The galaxy presents as a spiral type, exhibiting a prominent disk structure. Spiral arms are clearly visible, exhibiting a two-armed structure. The arms appear moderately wound and extend outwards from the central bulge region. The galaxy appears to be significantly inclined. The central bulge appears to be of small to moderate size relative to the overall disk. There is evidence of a possible bar structure, though somewhat difficult to resolve. The disk shows a slight blueness, potentially indicating ongoing star formation. There are possible minor disturbances within the disk, but no major mergers or significant tidal features can be observed.
