The galaxy presents as a somewhat elongated, disk-like structure, consistent with an elliptical morphology that is not perfectly circular when viewed from our perspective. Its color profile appears yellowish-white in the core, suggesting an older stellar population. There is little evidence of active star formation, and therefore, the galaxy probably has a low specific star formation rate. The apparent smoothness of the galaxy indicates that there is very little dust obscuration, or any signs of recent major merger events. However, there is some slight asymmetry that may indicate minor disturbance of this galaxy. The overall luminosity suggests the galaxy is relatively massive.
