The galaxy presents as a relatively face-on spiral type, with hints of a barred structure. A central bulge dominates the visual appearance, diminishing towards a diffuse disk. There are hints of spiral arm structure, though these are not particularly well defined. The bulge appears smooth, suggesting an older stellar population. There are no significant signs of recent or ongoing major mergers or strong tidal disturbances. The overall color appears to be intermediate between the blue of actively star-forming galaxies and the red of quiescent ellipticals.