The galaxy appears as a relatively small, elongated, disk-shaped object. It is likely an elliptical galaxy with a smooth, featureless profile, and possesses a significant red shift. A slight blue hue is detected at one end, suggesting possible lower metallicity or younger stars. There is no obvious central bulge or distinct spiral arm structure visible, nor are there signs of a currently active galactic nuclei.

The absence of strong color variations or significant dust lanes further suggests a relatively uniform stellar population with minimal ongoing star formation. Given the estimated distance, this galaxy is considered to be a massive object, even though it is not very active.
