The galaxy presents as a relatively smooth, elliptical-like object. It exhibits a concentrated central bulge which is a yellow, signifying older stellar populations. There is a smaller region to the lower right with similar color properties, it is unclear if this is a nucleus or a tidal feature. The overall structure suggests a system that has largely exhausted its supply of gas for star formation and is dominated by an older stellar population. There is no clear dust lane or significant signs of active star formation or spiral arm structure in the visible light data. The morphology appears close to spheroidal. It is possible this is a merging event with an older stellar population, which would explain the secondary grouping.
