The galaxy presents as a fairly smooth, elliptical-like object with a concentrated central bulge. It exhibits a golden hue, suggesting a population of older stars with lower rates of star formation. The shape is elongated, appearing somewhat in between a perfect circle and a cigar shape. There are no obvious signs of tidal disturbances or ongoing mergers, though subtle asymmetries are potentially present. The galaxy's color indicates significant presence of redder stellar populations.
