The galaxy presents as a centrally concentrated elliptical, with a smooth, diffuse profile, appearing quite luminous in the central region. The overall shape is slightly elongated with an axis ratio of roughly 5:6. The color appears to be dominated by light in the redder part of the spectrum, with a hint of yellow in the core, which is indicative of an older stellar population. There is little evidence of any spiral arm structure or significant dust lanes. The galaxy shows signs of only minor disturbances. Based on these morphological features and redshift, this galaxy can be considered to be relatively massive.
