The observed galaxy presents as a somewhat smooth, centrally concentrated object. It exhibits an overall elliptical morphology, appearing more "in between" round and elongated rather than distinctly circular or cigar-shaped. The light distribution suggests a substantial spheroidal component with a fairly homogeneous, diffuse structure. There is an indication of potential tidal disturbances in the galactic structure. The galaxy's color gradient suggests a population of older stars, with less ongoing star formation. The light from the core seems to be from an active galactic nucleus, although this can not be said for certain with only an image. 
