The galaxy presents a generally smooth, elliptical morphology. The light distribution is centrally concentrated with a gradual falloff in intensity moving outwards from the core.  A slight ellipticity is discernible, giving it a somewhat flattened appearance.  The dominant color is yellowish-white in the central region, suggesting an older stellar population. There is a hint of bluer light around the perimeter of the galaxy, suggesting that there could still be a very small amount of star forming activity in the galaxy, but it could also be an artifact of the observation. There is no evidence of spiral arms, dust lanes, or other distinct features. No obvious signs of interaction or merging are observed.
