The galaxy presents as a relatively smooth, centralized luminosity profile with minimal discernible features. There is a slight elongation observable, appearing to be more "in between" round and cigar shaped rather than distinctly round. The galaxy is primarily a singular object. There is no evidence of significant tidal disturbances or merging activity. Color gradients indicate a centrally concentrated older stellar population. There is also a slight indication of disk or spiral features, but mostly smooth.
