The galaxy presents as a relatively compact and luminous object. Its morphology appears largely smooth, with a generally rounded shape and only subtle deviations from perfect symmetry. There is a slight elongation, but no strong bar or spiral arm structure is readily apparent. Color gradients indicate a generally older stellar population, with a redder hue. There is a faint hint of bluer light concentrated in the central region. There are no prominent tidal features or signs of major ongoing mergers detected.
