The galaxy appears as a relatively smooth, elliptical or lenticular object. Its light is centrally concentrated, with a gradual decrease in surface brightness outward from the core. The color is generally consistent across the galaxy, trending toward the redder end of the spectrum, suggestive of an older stellar population with lower levels of on-going star formation. There is no evidence of a distinct disk structure, spiral arms, or significant dust lanes. The object exhibits a high degree of rotational symmetry, with no obvious signs of tidal disturbances or ongoing merger activity. There is a slight chance of a minor merging event.
