The galaxy presents as an elliptical morphology, with a smooth and concentrated light profile. The central region is bright, with the light appearing to dissipate gradually towards the edges. The color index suggests a population of older stars; with more light emitted in the redder bands than the blue bands. There is no apparent spiral arm structure nor significant dust lanes visible. The galaxy exhibits no signs of major interaction or merging events, showing a well-defined, undisturbed form. The overall round appearance is relatively smooth, with only minor deviations from perfect elliptical symmetry.
