The galaxy appears to be a relatively smooth, lenticular or elliptical galaxy at an approximate distance indicated by a redshift of z=0.18. The galaxy's light profile is concentrated toward the center, and the object presents as being somewhat oblate with a slight ellipticity. The galaxy's core is yellowish-orange, indicative of an older stellar population. There are little, if any, prominent spiral arms. The overall structure suggests a lack of significant ongoing star formation, and no merger events appear to be actively occurring. The galaxy seems to be relatively isolated.
