The galaxy appears to be elliptical or lenticular in morphology, exhibiting a generally smooth light distribution. There is a central bulge that is clearly visible, with the light intensity decreasing as you move outwards. The galaxy appears to be fairly undisturbed, showing no major signs of tidal distortions or ongoing mergers. The color index suggests a population of older stars; it is unlikely to be actively forming many new stars at this time. The shape of the galaxy appears to be somewhere between round and elliptical. There is no apparent spiral arm structure or dust lanes visible. There is possibly a very faint halo surrounding the galaxy.
