The galaxy presents as a spiral type, exhibiting a clear disk structure. Faint spiral arm features are present, though not sharply defined. A bar structure appears to cross the central region of the galaxy, though somewhat subtle. The bulge component appears moderately sized, blending smoothly into the disk. The galaxy displays a relatively high inclination, showing it to be close to edge-on. There are no obvious signs of significant tidal disturbances or ongoing major merging activity, though a slight asymmetry may hint at a minor interaction.
