The galaxy presents as a somewhat smooth structure, but with subtle features. The primary component appears elliptical in form, with an approximate projected half-light radius around 7 kpc. The galaxy exhibits a concentration of light towards the center.

There is evidence of substructure and/or possible tidal disturbances around the main body of the galaxy. These seem to manifest as slightly asymmetrical extensions, indicating the possibility of a past minor merger or interaction. A faint disk-like structure cannot be ruled out, but is not clearly defined. There is no clear evidence of strong recent star formation. The galaxy color is consistent with a relatively old stellar population.