The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution appears largely elliptical, with little to no evidence of spiral arms or a distinct disk. The overall color is a slightly yellow-white hue, suggestive of a moderate population of older stars. There may be some regions of bluer light indicative of recent star formation, but these are not particularly pronounced. The galaxy shows no obvious signs of a major ongoing merger or significant tidal disturbances. There appears to be a central bright region, possibly a core or bulge component. The size of the galaxy is relatively small.