The object presents as a relatively small, faint galaxy. It exhibits a largely smooth morphology with a concentrated central bulge that is bright white in color. The outer regions are less defined, appearing more diffuse. There may be some evidence of faint spiral structure, or simply an extended disk but this is not as prominent. No significant dust lanes or regions of intense star formation are readily apparent. Based on the red color index, this galaxy appears to host an older stellar population with a low star-formation rate. The light is relatively symmetrical indicating the galaxy may be undisturbed. There are no obvious signs of recent or ongoing merger activity or tidal disturbances.
