The galaxy presents with an elliptical morphology, appearing as an elongated spheroid. There is a smooth, dominant central bulge. The light distribution suggests a concentrated nucleus.

There is evidence of tidal disturbances that suggest a potential interaction or merger in progress. Observed is a faint tidal tail, which is a streaming feature, to one side. The main body shows some irregularities in its shape, which may also be related to gravitational interactions. 

It has an intermediate color profile, appearing neither strongly blue nor red. Some regions show hints of bluer patches which could be due to younger stars or recent star forming activity, although this is faint.