The galaxy presents an overall elliptical morphology with a high degree of central concentration, indicating a relatively smooth light distribution. There is little evidence of spiral arm structure or significant dust lanes within the galaxy. Its color appears generally red, suggesting an older stellar population, lower rates of ongoing star formation and/or a significant dust component. The shape shows a slight deviation from perfectly circular. There appear to be no visible disturbances attributable to recent mergers or interactions with other galaxies. The major axis has an approximate estimated length of 10 kiloparsecs, while it's redshift is around 0.13. The light profile appears well-fit by a Sersic profile. 
