The galaxy presents as a spiral galaxy, viewed at an oblique angle, exhibiting a significant degree of disk inclination relative to our line of sight. This near edge-on perspective obscures detailed observation of spiral arm structure, however there appears to be a bulge. The axial ratio suggests a flattened disk morphology. Light distribution is concentrated centrally, indicative of a substantial bulge component. The colour index, judging by the colour image, suggests a spectral type with a relatively old stellar population, though bluer areas can also be seen. There is a minor disturbance present; the asymmetry of light distribution suggests either tidal interaction, possibly due to an ongoing or recent minor merger, or internal asymmetries in star formation activity, as hinted by blue colour in some areas of the disk. There appears to be some smooth structure to the galaxy overall.
