The galaxy appears to be undergoing a merger event. It exhibits a generally smooth morphology with a dominant central bulge. There is evidence of a secondary, smaller concentration of light possibly a tidal tail or second smaller bulge. The galaxy shows an elliptical shape, with hints of disturbance in its outer regions, possibly indicating ongoing gravitational interactions. The overall color appears to be somewhat redder, suggesting an older stellar population with a very low star formation rate. The galaxy exhibits an extended halo of light.
