The galaxy presents as a generally smooth object. A significant portion of the galaxy's light is concentrated in a central region, likely the galactic bulge. The shape is predominantly elliptical, although there may be a slight elongation observable. It does not appear to exhibit any major disturbances indicative of recent or ongoing mergers, but there may be very minor tidal disturbances. The outer regions of the galaxy appear fainter and are less defined compared to the central bulge. There does not appear to be a lot of star forming regions within this galaxy.
