The galaxy presents as a smooth, elongated structure, possibly an elliptical or lenticular galaxy viewed at an angle. It appears to be dominated by an older stellar population, indicated by the yellowish-orange hue, which is consistent with lower star formation activity. There is no obvious spiral arm structure or dust lanes visible. There are no signs of major disturbances such as tidal tails or other obvious signs of a recent major merger. The galaxy exhibits a moderately compact core, with a diffuse halo extending outwards. There might be an indication of a minor disturbance. 
