The galaxy presents as a single, relatively smooth object. Its morphology is generally elliptical in nature, with a high degree of central concentration of light. There are no obvious spiral arm structures present. The galaxy appears to be a yellowish-white color.

The estimated half-light radius suggests the galaxy is a reasonably extended object. The spectral energy distribution indicates that the galaxy is relatively massive, and exhibits ongoing star formation, however the specific star formation rate shows that it is not a particularly vigorous star former. There appears to be no major ongoing merger events, but there are signs of minor gravitational disturbance.
