The galaxy presents as a relatively compact structure, approximately 8 kpc across. Its overall morphology suggests an elliptical or lenticular type. The light distribution appears smooth, lacking prominent spiral arms or a well-defined disk. The object is generally round in appearance, with minimal elongation. There is a noticeable concentration of light toward the central region, indicating a bulge. Faint, diffuse emission extends outwards from the core.

There is evidence of interaction and potentially, a recent or ongoing merger event. The galaxy exhibits some irregular features and asymmetries in its outer regions, indicating a disturbance in its overall structure. This disturbance could be due to gravitational interactions with another galaxy. It is difficult to tell if this merging is recent or further in the past. The redder colors also suggests that this galaxy is quiescent. Overall the galaxy is consistent with a spheroidal galaxy which has experienced a recent gravitational interaction.
