The galaxy presents as an elliptical-type galaxy, exhibiting a generally smooth and concentrated light profile. Its morphology is largely spheroidal, displaying high degree of central concentration. There may be a subtle indication of minor tidal interaction to the surrounding galaxy, but not enough to consider this to be considered an active merging galaxy. The luminosity is moderate, typical of a massive galaxy. Its color appears generally redder than typical for spiral galaxies, suggesting an older stellar population and lower ongoing star formation rate.
