The galaxy presents as a fairly concentrated, elliptical morphology with a smooth overall light distribution. There is a hint of deviation from perfect ellipticity but this may be due to it appearing to be in between round and elliptical. It is also possible this may be due to minor disturbances. The light appears to be dominated by older stellar populations, exhibiting a yellowish-red hue, suggesting relatively low ongoing star formation. No prominent spiral arms or disk-like structures are discernible. The galaxy exhibits a red shift of about 0.2 indicating that it is an older, distant object. The galaxy appears to be isolated, with no obvious signs of major interactions or ongoing merger activity with other galaxies nearby. 
