The galaxy presents as a relatively compact object. It is characterized by a flattened, somewhat elongated shape, appearing more cigar-shaped than circular. There is evidence of internal structure, potentially indicating a disk component, although this is not sharply defined. The overall texture appears relatively smooth, suggesting an older stellar population. There are no prominent signs of active star formation regions, nor indications of significant tidal disturbances or ongoing major mergers. It exhibits a color gradient, with a redder core, and bluer color in the edges of the disk.
