The galaxy appears to be relatively small and compact, exhibiting a central bright core. The overall shape is somewhat elliptical, but not perfectly round; it presents a more irregular appearance. There are hints of disturbed features in the galactic structure. The light distribution suggests there might be some disk like components present. There also appears to be possible merging or tidal disturbances that is suggested in the outskirts of the galaxy. The color gradients indicate a complex stellar population, with bluer regions potentially indicating younger stars or ongoing star formation.