The galaxy presents as a relatively smooth, elliptical structure. Its light distribution appears centrally concentrated with a gradual falloff towards the edges. The color profile is generally red, suggesting an older stellar population with a low rate of on-going star formation. There is evidence of some structural disturbance which is likely due to a past merger or tidal interaction. It has a fairly high degree of roundness and appears to have a high mass. Overall, it is an evolved galaxy currently not experiencing significant star formation.
